NGC 5275
NGC 5275 is a lenticular galaxy in the constellation Canes Venatici about 597 million ly from Earth. It spans roughly 150,000 ly, about 1.5 times the width of our Milky Way. It is receding from us at about 1,395 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 597 million ly from home, you are seeing NGC 5275 as it looked roughly 597 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 5282Elliptical33 million ly
apartNGC 5277Barred spiral42 million ly
apartIC 4300Elliptical52 million ly
apartIC 4334Elliptical58 million ly
apartNGC 5441Barred spiral72 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).