NGC 195
NGC 195 is a spiral galaxy in the constellation Cetus about 228 million ly from Earth. It spans roughly 81,000 ly, about 81% of our Milky Way's width. It is receding from us at about 4,918 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 228 million ly from home, you are seeing NGC 195 as it looked roughly 228 million years ago. The photons left before that much of history had passed, and are only now reaching us. This distance is estimated from the galaxy's redshift, so the lookback time is approximate.
apartIC 16Lenticular19 million ly
apartNGC 321Elliptical24 million ly
apartNGC 341Barred spiral25 million ly
apartNGC 277Elliptical29 million ly
apartNGC 345Spiral30 million ly
apart
Source: structural data (position, morphology, brightness, redshift) from OpenNGC (CC BY-SA). Recession velocity from RC3 (de Vaucouleurs et al. 1991, via NASA/HEASARC, public domain). Distance computed by gravityfinder from redshift via Hubble's law (H0 = 70 km/s/Mpc).