The galaxy presents as a likely interacting system, potentially in the early stages of a merger event. Morphologically, the system appears to comprise two distinct components. The larger component exhibits a centrally concentrated light profile consistent with an elliptical or lenticular galaxy. It possesses a smooth appearance, but may show some disturbances in the outer regions. The smaller component appears more disturbed, with a less-defined structure, and it may also be tidally interacting with the larger component. The overall color is slightly redder, indicating a relatively older stellar population and lower rate of star formation. The apparent size is relatively small suggesting a moderate distance. There may be a hint of tidal features present, but the image resolution limits definitive confirmation.
