NGC 3451
NGC 3451 is a spiral galaxy in the constellation Leo Minor about 62 million ly from Earth. It spans roughly 30,000 ly, about 30% of our Milky Way's width. The light reaching us tonight left it about 62 million years ago.
Illustration from its catalogued shape, not a photograph
Because its light is 62 million ly from home, you are seeing NGC 3451 as it looked roughly 62 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 3418Lenticular3.8 million ly
apartNGC 3400Barred spiral4.0 million ly
apartNGC 3414Lenticular5.5 million ly
apartNGC 3437Spiral5.9 million ly
apartNGC 3277Spiral6.6 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).