NGC 4379
NGC 4379 is an elliptical galaxy in the constellation Coma Berenices about 48 million ly from Earth. It spans roughly 26,000 ly, about 26% of our Milky Way's width. It is receding from us at about 1,056 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 48 million ly from home, you are seeing NGC 4379 as it looked roughly 48 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 4394Barred spiral2.6 million ly
apartIC 3065Lenticular2.9 million ly
apartNGC 4336Lenticular3.3 million ly
apartIC 3356Irregular3.4 million ly
apartIC 3465Elliptical3.6 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).