NGC 1808
NGC 1808 is a spiral galaxy in the constellation Columba about 47 million ly from Earth. It spans roughly 74,000 ly, about 74% of our Milky Way's width. It is receding from us at about 1,014 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 47 million ly from home, you are seeing NGC 1808 as it looked roughly 47 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 1679Barred spiral6.0 million ly
apartNGC 1792Barred spiral10 million ly
apartNGC 1531Elliptical11 million ly
apartNGC 1510Lenticular11 million ly
apartIC 2041Lenticular12 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).