NGC 1087
NGC 1087 is a spiral galaxy in the constellation Cetus about 71 million ly from Earth. It spans roughly 61,000 ly, about 61% of our Milky Way's width. It is receding from us at about 1,508 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 71 million ly from home, you are seeing NGC 1087 as it looked roughly 71 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 955Spiral5.0 million ly
apartIC 225Elliptical6.6 million ly
apartNGC 963Irregular7.0 million ly
apartNGC 941Spiral7.4 million ly
apartNGC 1022Barred spiral8.2 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).