IC 4189
IC 4189 is a spiral galaxy in the constellation Canes Venatici about 224 million ly from Earth. It spans roughly 81,000 ly, about 81% of our Milky Way's width. It is receding from us at about 4,810 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 224 million ly from home, you are seeing IC 4189 as it looked roughly 224 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 4956Lenticular3.9 million ly
apartNGC 4914Elliptical9.4 million ly
apartNGC 4868Spiral9.6 million ly
apartNGC 4846Barred spiral14 million ly
apartIC 3892Lenticular17 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).