NGC 4696D
NGC 4696D is a lenticular galaxy in the constellation Centaurus about 121 million ly from Earth. It spans roughly 48,000 ly, about 48% of our Milky Way's width. It is receding from us at about 2,590 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 121 million ly from home, you are seeing NGC 4696D as it looked roughly 121 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 4603Spiral3.4 million ly
apartNGC 4661Elliptical4.1 million ly
apartNGC 4930Barred spiral6.2 million ly
apartNGC 4603DSpiral7.5 million ly
apartNGC 4696ABarred spiral11 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).