The galaxy presents a generally smooth morphology, with a dominant, centrally concentrated bulge. The light distribution suggests a primarily spheroidal shape, appearing mostly round. There is some visual evidence of disturbances; what could be multiple cores or tidal tails suggest an ongoing or recent interaction with another galaxy or merging event. The galaxy exhibits a color gradient, appearing bluer in the outer regions, suggesting ongoing star formation in those regions. There is not a clearly defined disk structure, and any spiral arm presence is either absent or obscured. Based on the overall characteristics, the galaxy may be classified as an elliptical galaxy undergoing a merger event.
