The galaxy appears to be a luminous, centrally concentrated system with an ellipsoidal morphology. Its overall color is yellowish-white, suggesting a dominant population of older stars. There is a possible disk-like component, though the prominence is not significant. The galaxy exhibits some signs of disturbances in the form of clumps and a warped appearance suggesting potential tidal interactions or a recent merger event. The estimated size is several kiloparsecs. Star formation appears to be present, but at a suppressed rate.
