NGC 4108
NGC 4108 is a spiral galaxy in the constellation Draco about 117 million ly from Earth. It spans roughly 56,000 ly, about 56% of our Milky Way's width. It is receding from us at about 2,502 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 117 million ly from home, you are seeing NGC 4108 as it looked roughly 117 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 spiral3.7 million ly
apartNGC 4034Spiral7.6 million ly
apartNGC 4512Lenticular8.6 million ly
apartNGC 4128Lenticular8.8 million ly
apartNGC 4441Lenticular9.6 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).