The galaxy presents as a complex system, potentially undergoing a merger or interaction. The primary component exhibits a somewhat smooth, elliptical morphology, with a concentrated central bulge that appears yellow-white in color. This suggests a population of older stars. Extending from this core are several distinct components. To the left of the galaxy's core there appears a reddish, seemingly detached, structure. To the right, there are hints of another component. Overall, there is little indication of prominent spiral arms or significant dust lanes, however, signs of distortion are present and the shapes appear distorted from the merger.
