NGC 4109
NGC 4109 is a spiral galaxy in the constellation Canes Venatici about 327 million ly from Earth. It spans roughly 67,000 ly, about 67% of our Milky Way's width. The light reaching us tonight left it about 327 million years ago.
Illustration from its catalogued shape, not a photograph
Because its light is 327 million ly from home, you are seeing NGC 4109 as it looked roughly 327 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 4288ALenticular23 million ly
apartIC 2987Barred spiral26 million ly
apartNGC 4226Barred spiral27 million ly
apartNGC 4392Lenticular28 million ly
apartNGC 4232Barred spiral30 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).