Before Galileo started looking at the sky through his telescope, the only permanent things in the sky that were not points were the Sun, the Moon, and the Milky Way (unless you could see the Magellanic Clouds!). And the points - stars - did not change their relative positions, the Moon always looked the same, as did the Milky Way (and the Magellanic Clouds). Sometimes the Sun got spots on it, and the full Moon got dim, and even turned a beautiful reddish-orange (but otherwise looked the same); very rarely (only during a total eclipse of the Sun) a lovely pearly glow could be seen around the Sun (or was it the Moon?). Some of the stars did seem to change a bit in brightness, and one or two got so faint they disappeared for a while (but they always came back). Occasionally there was a comet, and very rarely a 'guest star'.
Except, of course, for the five planets - Mercury, Venus, Mars, Jupiter, and Saturn; they wandered around the sky, but in a way that seemed to fit a pattern.
The pinnacle of pre-telescopic astronomy (at least in Europe) was Tycho Brahe's star catalogue and meticulous sets of records of the positions of the planets. Not surprisingly, they are wholly quantitative, i.e. 'just' sets of numbers, no 'a little bit to the west of', or 'close to'. In fact, Tycho even estimated what we'd today call the uncertainty, or error, in his quantitative data; however, his estimates turned out, upon later analysis, to have been somewhat under-estimates (among other things, there was an unrecognised systematic error in his star catalogue; systematic errors are the bane of an astronomer's life!).
Once telescopes were used to observe the sky, quite a few objects were seen to be more than just points, so observational astronomy began to include some drawings, or paintings, qualitative data in other words (and not just maps of the Moon!). In fact, there really was no way to record what we today call 'extended objects' except by drawing them (well, 'word pictures' were possible, but a rather poor alternative).
That is until photography began to be used in astronomy. Then astronomical observations became a lot less subjective, and quantitative analyses of extended objects - galaxies (as we call them today), nebulae (of various kinds) - began to become common. However, quantitative analyses of this kind are often quite tedious, especially if you have to do all the calculations by hand!
Starting around the 1960s two revolutions began to hit observational astronomy, CCDs and computers; fast forward to the 21st century, and everything is now quantitative.
When you look at an Astronomy Picture of the Day which comes from the Hubble, Swift, Herschel, Fermi, XMM-Newton, Planck, one of the Very Large Telescopes in Chile, one of the Kecks (in Hawaii), SDSS, or even an amateur's backyard telescope ... what looks like a picture, or image, or photograph, isn't. What it is is a representation of rather a lot of data, and nearly always involves considerable processing of the outputs from whatever instruments or detectors were used (done by computers, of course). You could take the very same data, process it in a different way, and produce an image which looks quite different! We are all probably used to 'false colour images', but you'd be surprised at how differently the very same data can be made to appear ... yet its status as an astronomical observation is exactly the same.