NGC 4226
NGC 4226 is a barred spiral galaxy in the constellation Canes Venatici about 338 million ly from Earth. It spans roughly 110,000 ly, about the width of our Milky Way. It is receding from us at about 7,238 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 338 million ly from home, you are seeing NGC 4226 as it looked roughly 338 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 4231Lenticular8.4 million ly
apartNGC 4392Lenticular11 million ly
apartNGC 4288ALenticular13 million ly
apartNGC 4109Spiral27 million ly
apartIC 731Barred spiral35 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).