NGC 4298
NGC 4298 is a spiral galaxy in the constellation Coma Berenices about 53 million ly from Earth. It spans roughly 39,000 ly, about 39% of our Milky Way's width. It is receding from us at about 1,122 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 53 million ly from home, you are seeing NGC 4298 as it looked roughly 53 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 4436Lenticular2.8 million ly
apartNGC 4344Lenticular3.0 million ly
apartVirgo AElliptical3.0 million ly
apartIC 3081Elliptical3.0 million ly
apartNGC 4459Lenticular3.2 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).