The galaxy presents as an elliptical morphology, characterized by a centrally concentrated bulge. It exhibits a smooth appearance with no discernible spiral arms or distinct features suggestive of active star formation regions. The color profile indicates a dominant population of older stars, as evidenced by the redder hues concentrated in the central bulge and extending outward. The outer regions appear slightly bluer, potentially indicating a younger stellar population or some residual star formation activity. The overall shape is somewhat elongated. There is no indication of a major ongoing merger event or significant tidal disturbances. The galaxy exhibits a consistent, smooth light distribution.
