NGC 2591
NGC 2591 is a spiral galaxy in the constellation Camelopardalis about 62 million ly from Earth. It spans roughly 53,000 ly, about 53% 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 2591 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 2655Lenticular4.2 million ly
apartNGC 2748Barred spiral7.7 million ly
apartNGC 2985Spiral8.0 million ly
apartNGC 3403Barred spiral10 million ly
apartNGC 2760Elliptical11 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).