The galaxy presents a generally smooth and elliptical morphology. There is evidence of a slight colour gradient from the center outwards. The central region displays a yellowish hue, suggesting an older stellar population. Moving outward, there is a slight shift to a bluer hue which is indicative of recent, or ongoing, star formation, potentially a spiral disk. Based on its somewhat disturbed appearance, it is likely undergoing a merger with a smaller satellite galaxy. There appears to be some tidal features disrupting the primary galaxy which may have been caused by the interaction.
