The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. It exhibits a concentrated central bulge that gradually diffuses outwards, diminishing into the surrounding space. The color profile suggests an aging stellar population with the presence of older stars. There are no indications of active spiral arms or significant dust lanes. There is a lack of any prominent star-forming regions. The shape shows a high degree of circularity. There is no visual evidence of any recent or ongoing major merger activity, but there is a slight asymmetry in the outer halo, which could indicate a very minor past disturbance. The overall impression is of a well-established, relatively quiescent galaxy.
