NGC 4132
NGC 4132 is a spiral galaxy in the constellation Coma Berenices about 186 million ly from Earth. It spans roughly 62,000 ly, about 62% of our Milky Way's width. It is receding from us at about 4,069 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 186 million ly from home, you are seeing NGC 4132 as it looked roughly 186 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 4196Lenticular5.2 million ly
apartNGC 4175Barred spiral5.8 million ly
apartNGC 4131Lenticular6.1 million ly
apartNGC 4185Barred spiral6.5 million ly
apartNGC 4169Lenticular10 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).