The galaxy presents as a centrally concentrated system with a smooth overall light distribution. There is a subtle elongation apparent, suggesting a disc-like component but no clear spiral arm structure is visible. The central region is bright and unresolved, possibly indicative of an older stellar population. Fainter, bluer light is discernible throughout the main body of the galaxy, with some hint of patchy star formation activity. There may be some minor tidal disturbances present along one side, potentially caused by a minor merger. The galaxy appears relatively isolated.
