IC 467
IC 467 is a spiral galaxy in the constellation Camelopardalis about 96 million ly from Earth. It spans roughly 55,000 ly, about 55% of our Milky Way's width. It is receding from us at about 2,057 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 96 million ly from home, you are seeing IC 467 as it looked roughly 96 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 2732Lenticular9.0 million ly
apartIC 469Spiral9.3 million ly
apartNGC 2300Elliptical11 million ly
apartNGC 2268Barred spiral11 million ly
apartIC 455Lenticular12 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).