The galaxy presents as an elliptical or lenticular system, displaying a smooth, centrally concentrated morphology. The galaxy exhibits a noticeable color gradient, with a yellowish core indicating an older stellar population and potentially a larger presence of dust. A fainter, bluer halo is visible, suggesting some level of ongoing star formation. The object displays an intermediate roundness. There is no visual evidence of a major merger event, although the subtle irregularity may indicate a minor disturbance or past interaction. The galaxy is estimated to be of substantial mass, with moderate star formation activity relative to its mass. The inferred size is substantial, indicating a relatively large galaxy.
