NGC 4886
NGC 4886 is an elliptical galaxy in the constellation Coma Berenices about 297 million ly from Earth. It spans roughly 69,000 ly, about 69% of our Milky Way's width. It is receding from us at about 6,345 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 297 million ly from home, you are seeing NGC 4886 as it looked roughly 297 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.
apartIC 3957Elliptical1.6 million ly
apartNGC 4889Elliptical3.5 million ly
apartIC 4133Elliptical4.4 million ly
apartNGC 4841BElliptical6.5 million ly
apartNGC 4828Lenticular6.5 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).