NGC 4276
NGC 4276 is a spiral galaxy in the constellation Virgo about 123 million ly from Earth. It spans roughly 48,000 ly, about 48% of our Milky Way's width. It is receding from us at about 2,628 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 123 million ly from home, you are seeing NGC 4276 as it looked roughly 123 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 4191Lenticular3.6 million ly
apartNGC 4249Elliptical5.0 million ly
apartNGC 4257Spiral5.2 million ly
apartNGC 4281Lenticular5.2 million ly
apartNGC 4264Lenticular7.3 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).