The galaxy presents as a roughly elliptical, though not perfectly spherical, structure. It exhibits a smooth and centrally concentrated light profile, suggesting a relatively old stellar population with minimal dust obscuration. The core region displays a yellowish-white hue, indicative of older stars, and a diminished rate of current star formation. No distinct spiral arms or bar structures are visible. The outer regions fade gradually into the background, showing no signs of major tidal disturbances or ongoing merger activity. The overall appearance points toward a galaxy that is largely quiescent in terms of recent or ongoing interactions or significant starburst events.
