IC 499
IC 499 is a spiral galaxy in the constellation Camelopardalis about 88 million ly from Earth. It spans roughly 48,000 ly, about 48% of our Milky Way's width. It is receding from us at about 1,883 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 88 million ly from home, you are seeing IC 499 as it looked roughly 88 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 2300Elliptical2.8 million ly
apartIC 469Spiral10 million ly
apartNGC 2732Lenticular11 million ly
apartIC 512Spiral13 million ly
apartIC 467Spiral13 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).