The galaxy appears as a somewhat diffuse and luminous object, exhibiting a primarily smooth morphology. The overall color profile suggests a population dominated by older stars, giving it a reddish-yellow hue. The galaxy seems relatively round in shape, showing minimal deviations from spherical symmetry. There are no prominent spiral arms or a well-defined disk visible. Hints of a possible interaction or merger are present with a possible merging event with another object, which could be a smaller galaxy. Overall, it is an elliptical galaxy likely undergoing a merger.
