NGC 3799 is a barred spiral galaxy located in the constellation Leo.

Its speed relative to the cosmic microwave background is 3,659 ± 24 km/s, which corresponds to a Hubble distance of 54.0 ± 3.8 Mpc (~176 million ly).

[3] Halton Arp describes these as an example of galaxies by presenting a bridge of matter between them and having a high surface gloss.

[2] To date, a non-redshift measurement gives a distance of approximately 47 Mpc (~153 million ly).

Note, however, that it is with the average value of independent measurements, when they exist, that the NASA/IPAC database calculates the diameter of a galaxy.