The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution. There is a bright, concentrated core region with a gradual decrease in luminosity towards the outer regions. The object appears to be moderately elongated. There is no readily apparent spiral structure or significant dust lane obscuration. The color profile is primarily in the redder wavelengths, indicative of an older stellar population, although a small, slightly bluer region is noticeable on one edge, suggesting possible minor star formation. Overall, the galaxy appears to be a relatively evolved, quiescent system.
