IC 1790
IC 1790 is a spiral galaxy in the constellation Aries about 172 million ly from Earth. It spans roughly 41,000 ly, about 41% of our Milky Way's width. It is receding from us at about 3,597 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 172 million ly from home, you are seeing IC 1790 as it looked roughly 172 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.
apartNGC 871Barred spiral6.7 million ly
apartIC 195Lenticular12 million ly
apartIC 196Spiral12 million ly
apartIC 1774Spiral13 million ly
apartNGC 876Spiral13 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).