The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent merger event. The primary body of the galaxy appears diffuse, with a smooth light profile indicative of an elliptical galaxy. There are features that disrupt the smooth profile of the galaxy, likely tidal tails or other remnants of the merger. A significant concentration of light is seen in the central region with some yellow to red tint, suggesting an older stellar population. A fainter, more diffuse bluish component is also present, hinting at some ongoing star formation, albeit at a moderate rate. The galaxy's overall shape is roughly elliptical but with notable deviations, suggesting a system in transition.
