NGC 6630
NGC 6630 is an elliptical galaxy in the constellation Pavo about 125 million ly from Earth. It spans roughly 30,000 ly, about 30% of our Milky Way's width. It is receding from us at about 2,646 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 125 million ly from home, you are seeing NGC 6630 as it looked roughly 125 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.
apartIC 4782Spiral20 million ly
apartIC 4797Elliptical21 million ly
apartIC 4821Spiral21 million ly
apartNGC 6305Elliptical22 million ly
apartNGC 6707Barred spiral22 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).