The galaxy appears as a relatively smooth, centrally concentrated object with a round morphology. The light distribution suggests a spheroidal shape. There are indications of a possible ongoing merger event, with a smaller, secondary luminous component closely interacting with the main galaxy body. The primary component exhibits an orange-red hue, suggesting a population of older, evolved stars. The apparent lack of blue color suggests a low rate of current star formation. Based on its overall appearance, this galaxy could be an elliptical galaxy or a spiral galaxy undergoing a merger that has disrupted its disk. It is likely a very massive galaxy. The irregular shape and disturbed morphology suggest a potentially complex evolutionary history.
