NGC 2227
NGC 2227 is a spiral galaxy in the constellation Canis Major about 107 million ly from Earth. It spans roughly 70,000 ly, about 70% of our Milky Way's width. It is receding from us at about 2,221 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 107 million ly from home, you are seeing NGC 2227 as it looked roughly 107 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 2212Lenticular11 million ly
apartNGC 2272Elliptical14 million ly
apartNGC 2211Lenticular15 million ly
apartNGC 2292Lenticular15 million ly
apartNGC 2293Lenticular16 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).