NGC 4247
NGC 4247 is a spiral galaxy in the constellation Virgo about 182 million ly from Earth. It spans roughly 53,000 ly, about 53% of our Milky Way's width. It is receding from us at about 3,944 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 182 million ly from home, you are seeing NGC 4247 as it looked roughly 182 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 4296Lenticular4.9 million ly
apartNGC 4246Spiral9.6 million ly
apartIC 768Spiral17 million ly
apartNGC 4334Spiral18 million ly
apartNGC 4012Spiral22 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).