NGC 4158
NGC 4158 is a spiral galaxy in the constellation Coma Berenices about 115 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 2,413 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 115 million ly from home, you are seeing NGC 4158 as it looked roughly 115 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 4529Spiral11 million ly
apartIC 3049Spiral11 million ly
apartIC 3365Irregular12 million ly
apartComa PinwheelSpiral12 million ly
apartNGC 4162Barred spiral13 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).