NGC 7250
NGC 7250 is a spiral galaxy in the constellation Lacerta about 54 million ly from Earth. It spans roughly 34,000 ly, about 34% of our Milky Way's width. It is receding from us at about 1,165 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 54 million ly from home, you are seeing NGC 7250 as it looked roughly 54 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 7332Lenticular17 million ly
apartNGC 7339Spiral19 million ly
apartNGC 7177Spiral22 million ly
apartIC 1420 NED02Spiral26 million ly
apartNGC 7241Barred spiral26 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).