NGC 1588
NGC 1588 is an elliptical galaxy in the constellation Taurus about 163 million ly from Earth. It spans roughly 60,000 ly, about 60% of our Milky Way's width. It is receding from us at about 3,458 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 163 million ly from home, you are seeing NGC 1588 as it looked roughly 163 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 1620Spiral5.1 million ly
apartNGC 1587Elliptical9.8 million ly
apartIC 363Elliptical11 million ly
apartNGC 1635Lenticular12 million ly
apartNGC 1638Lenticular12 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).