NGC 4592
NGC 4592 is a spiral galaxy in the constellation Virgo about 50 million ly from Earth. It spans roughly 60,000 ly, about 60% of our Milky Way's width. It is receding from us at about 1,176 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 50 million ly from home, you are seeing NGC 4592 as it looked roughly 50 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 4546Elliptical3.2 million ly
apartNGC 4517Spiral3.2 million ly
apartNGC 4691Lenticular4.0 million ly
apartNGC 4772Spiral4.4 million ly
apartNGC 4544Barred spiral4.8 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).