The galaxy presents a generally smooth and rounded morphology. Its light profile is centrally concentrated. There is an indication of a slight color gradient, with a reddish core transitioning to bluer outer regions. This may be due to older stellar populations dominating the core region, while younger, bluer stars are more prevalent in the outer parts of the galaxy. It is possible that the galaxy has undergone a minor interaction with a smaller object at some point in its history, although it does not appear to be currently undergoing any major merging activity. Given the overall smooth appearance, it could be classified as an elliptical galaxy.
