The galaxy presents as a moderately bright elliptical, exhibiting a smooth, relatively featureless morphology. Its color profile indicates a predominantly mature stellar population, with a higher concentration of redder light toward the core, indicative of older stars. The outer regions show a subtle shift toward bluer wavelengths, potentially suggesting some ongoing, albeit low-level, star formation. The overall shape is more of an oval, rather than a perfect sphere, with no obvious signs of tidal disturbances or recent major mergers. There is a suggestion of a faint disk, which is unusual given the older population. The galaxy appears to be relatively isolated in its immediate surroundings, though another galaxy is close by and may be merging. The general structure implies that the galaxy has a relatively high mass.
