The galaxy presents a generally smooth, rounded morphology. There is evidence of ongoing or recent merging activity, characterized by multiple distinct and bright regions. The galaxy shows an intermediate color profile, with a yellowish hue indicative of a mixed population of stars. There is no evidence of spiral arms or a clear disk component. The size appears relatively compact, with a somewhat concentrated light distribution. Overall, the galaxy appears as an elliptical, potentially undergoing interaction with a smaller system.