The galaxy presents a generally smooth, elliptical morphology with minimal discernible substructure. It exhibits a concentrated central bulge that dominates the overall luminosity profile, gradually fading into the outer regions. The color index suggests a population of older stars, consistent with an evolved stellar population. The galaxy displays a nearly circular isophotal shape, with no prominent tidal features or signs of recent major merger activity. There is no prominent dust lane and no sign of active star formation in the galaxy.
