The galaxy presents a morphology indicating a system undergoing or having undergone a significant interaction. The primary body displays a generally elliptical shape with a notable central concentration of luminosity. This core region exhibits a yellowish-white hue, potentially indicating an older stellar population. A distinct, elongated structure extends from the main body. This feature shows a more reddish tint, suggestive of dust lanes or regions of ongoing star formation. The system's overall structure indicates a substantial mass, given the apparent gravitational influence shaping its morphology. There's a secondary, less prominent component visible, slightly offset from the main body. Its reddish color suggests either a distinct population of older stars, or a region heavily obscured by dust. The overall structure, including the disturbances in morphology, points toward a potential merger event.
