The galaxy presents as a moderately luminous object, exhibiting a red-shifted spectrum. Its morphology appears to be largely smooth, but with some indication of disturbed or irregular features, possibly indicating a recent or ongoing interaction. The light distribution is dominated by a central component that is moderately red, suggesting an older stellar population. There are other less luminous, bluer areas around the galaxy, which may represent younger regions of star formation. The galaxy's overall shape appears somewhere in between round and elongated, with no obvious spiral arms or bar structure. This galaxy has an estimated mass on the order of 10^11 solar masses, and very low star formation activity.
