NGC 1719
NGC 1719 is a spiral galaxy in the constellation Orion about 194 million ly from Earth. It spans roughly 62,000 ly, about 62% of our Milky Way's width. It is receding from us at about 4,165 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 194 million ly from home, you are seeing NGC 1719 as it looked roughly 194 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 1740Elliptical11 million ly
apartNGC 1741BSpiral14 million ly
apartNGC 1683Spiral14 million ly
apartNGC 1741Spiral14 million ly
apartNGC 1713Elliptical15 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).