The galaxy appears as a single, relatively smooth, and concentrated object. Its overall shape is elliptical, appearing largely spheroidal with a high degree of circularity. The color profile suggests a greater concentration of older stars. There are no obvious spiral arm structures or significant dust lanes visible, indicating it is a relatively smooth galaxy with little to no star formation. There are no signs of significant tidal disturbances or ongoing mergers. There is some evidence of minor asymmetry within the central region, possibly indicating minor interactions, however, they are not prominent.
