IC 2209
IC 2209 is a barred spiral galaxy in the constellation Camelopardalis about 67 million ly from Earth. It spans roughly 16,000 ly, about 16% of our Milky Way's width. It is receding from us at about 1,413 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 67 million ly from home, you are seeing IC 2209 as it looked roughly 67 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 2654Barred spiral8.4 million ly
apartNGC 2768Elliptical11 million ly
apartNGC 2742Spiral12 million ly
apartNGC 2820ASpiral12 million ly
apartNGC 2820Barred spiral12 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).