NGC 3177
NGC 3177 is a spiral galaxy located in the constellation Leo. Its speed relative to the cosmic microwave background is 1,627 ± 22 km/s, which corresponds to a Hubble distance of 24.0 ± 1.7 Mpc. NGC 3177 was discovered by the German-British astronomer William Herschel in 1784.
The luminosity class of NGC 3177 is II and it has a broad HI line. It also contains regions of ionized hydrogen. According to the SIMBAD database, NGC 3177 has an active galactic nucleus.
To date, nine non-redshift measurements yield a distance of 27.722 ± 4.581 Mpc, which is within the distance values of Hubble.