NGC 4275
NGC 4275 is a spiral galaxy in the constellation Coma Berenices about 108 million ly from Earth. It spans roughly 27,000 ly, about 27% of our Milky Way's width. It is receding from us at about 2,307 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 108 million ly from home, you are seeing NGC 4275 as it looked roughly 108 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 4158Spiral16 million ly
apartNGC 4529Spiral19 million ly
apartNGC 4162Barred spiral19 million ly
apartNGC 4793Spiral21 million ly
apartIC 3298Barred spiral21 million ly
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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).