The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light distribution. Its overall color is yellowish-orange, indicating a dominant population of older stars and a lower rate of current star formation. The galaxy exhibits a nearly circular morphology, with a high degree of central concentration. There is no obvious evidence of spiral arm structure or significant dust lanes. The lack of distinct features suggests a well-mixed stellar population and a history of relatively quiescent evolution. There are slight indications of a minor disturbance event.
