NGC 3277
NGC 3277 is a spiral galaxy in the constellation Leo Minor about 66 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 1,460 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 66 million ly from home, you are seeing NGC 3277 as it looked roughly 66 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 3254Barred spiral2.8 million ly
apartNGC 3245ABarred spiral3.0 million ly
apartNGC 3245Lenticular4.1 million ly
apartNGC 3400Barred spiral4.5 million ly
apartNGC 3414Lenticular5.0 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).