The galaxy exhibits a complex morphology, potentially indicating an ongoing or recent merger event. The core region appears concentrated, with two brighter, somewhat unresolved components. The overall light distribution suggests an elliptical shape, but is noticeably disturbed. There are faint extended features surrounding the central components which may represent tidal tails or disrupted spiral arms. Colors range from a somewhat redder central region to bluer extended areas. This suggests a mix of older stellar populations centrally, and some regions of potentially active star formation in the outer regions. The system appears to be relatively massive.
