The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology, showing a somewhat rounded shape, with the isophotes appearing largely regular. The light profile suggests a possible spheroidal component dominating its structure, with no apparent spiral arms or a prominent disk visible in this imaging. The color index is moderate, appearing overall yellowish-white. This color is indicative of an older stellar population and reduced star formation. There is some evidence of interaction or tidal features.
