NGC 1517
NGC 1517 is a spiral galaxy in the constellation Taurus about 162 million ly from Earth. It spans roughly 46,000 ly, about 46% of our Milky Way's width. It is receding from us at about 3,644 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 162 million ly from home, you are seeing NGC 1517 as it looked roughly 162 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 363Elliptical18 million ly
apartNGC 1550Elliptical22 million ly
apartIC 366Elliptical24 million ly
apartNGC 1590Spiral25 million ly
apartIC 364Lenticular26 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).