NGC 4172
NGC 4172 is a spiral galaxy in the constellation Ursa Major about 434 million ly from Earth. It spans roughly 160,000 ly, about 1.6 times the width of our Milky Way. It is receding from us at about 9,274 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 434 million ly from home, you are seeing NGC 4172 as it looked roughly 434 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 4181Elliptical29 million ly
apartNGC 3846Barred spiral36 million ly
apartNGC 4187Elliptical41 million ly
apartNGC 4054 NED02Spiral44 million ly
apartNGC 4054 NED01Barred spiral45 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).