NGC 4108B
NGC 4108B is a spiral galaxy in the constellation Draco about 120 million ly from Earth. It spans roughly 46,000 ly, about 46% of our Milky Way's width. It is receding from us at about 2,575 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 120 million ly from home, you are seeing NGC 4108B as it looked roughly 120 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 4256Barred spiral4.2 million ly
apartNGC 4210Barred spiral6.9 million ly
apartNGC 4441Lenticular7.8 million ly
apartNGC 4512Lenticular9.1 million ly
apartNGC 4332Barred spiral9.8 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).