The galaxy presents as a relatively compact and smooth elliptical galaxy with a generally round morphology. There is no apparent evidence of spiral arms or a well-defined disk structure. The galaxy's color appears to be on the redder end, suggesting a population of older stars and a lower rate of ongoing star formation, though the galaxy does emit some light in the bluer wavelengths. There is a suggestion of minor disturbances or tidal features that may indicate a recent or ongoing interaction with another galaxy. The system might be in the process of a merger with another galaxy, or it could be a flyby.