NGC 3258D
NGC 3258D is a barred spiral galaxy in the constellation Antlia about 116 million ly from Earth. It spans roughly 67,000 ly, about 67% of our Milky Way's width. It is receding from us at about 2,722 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 116 million ly from home, you are seeing NGC 3258D as it looked roughly 116 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 3260Elliptical2.1 million ly
apartNGC 3281BElliptical2.5 million ly
apartIC 2584Lenticular3.7 million ly
apartNGC 3258CSpiral5.7 million ly
apartNGC 3281DBarred spiral7.0 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).