NGC 4899
NGC 4899 is a spiral galaxy in the constellation Virgo about 124 million ly from Earth. It spans roughly 73,000 ly, about 73% of our Milky Way's width. It is receding from us at about 2,623 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 124 million ly from home, you are seeing NGC 4899 as it looked roughly 124 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 4887Lenticular2.2 million ly
apartNGC 4897Barred spiral4.9 million ly
apartNGC 5044Elliptical9.4 million ly
apartNGC 5049Lenticular10 million ly
apartNGC 5077Elliptical10 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).