NGC 2199
NGC 2199 is a spiral galaxy in the constellation Mensa about 211 million ly from Earth. It spans roughly 140,000 ly, about the width of our Milky Way. It is receding from us at about 4,470 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 211 million ly from home, you are seeing NGC 2199 as it looked roughly 211 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 2150Spiral14 million ly
apartIC 2160Barred spiral18 million ly
apartNGC 1956Spiral24 million ly
apartIC 2103Spiral26 million ly
apartIC 2089Spiral27 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).