NGC 4250
NGC 4250 is a lenticular galaxy in the constellation Draco about 100 million ly from Earth. It spans roughly 54,000 ly, about 54% of our Milky Way's width. It is receding from us at about 2,032 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 100 million ly from home, you are seeing NGC 4250 as it looked roughly 100 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 4572Spiral6.8 million ly
apartNGC 4108ABarred spiral8.9 million ly
apartNGC 4128Lenticular9.8 million ly
apartNGC 4121Elliptical10 million ly
apartNGC 4513Lenticular11 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).