The galaxy presents as an elliptical or lenticular system, appearing largely smooth and featureless. Its morphology is elongated, displaying a shape intermediate between a perfect circle and a highly elongated form. The light profile indicates a centrally concentrated brightness that gradually diminishes towards the outer edges. The primary color appears reddish, possibly indicating an older stellar population and a lower rate of ongoing star formation. There is a strong suggestion of a possible minor disturbance, which may indicate a past interaction with another galaxy. The interaction does not seem to indicate a full merger, but a slight disruption may be present within the galaxy's structure.
