The galaxy appears to be an interacting system, showing signs of a possible merger in progress. The primary component presents a smooth, centrally concentrated morphology, possibly an elliptical galaxy. This suggests an older stellar population. The secondary component displays a more irregular structure. The presence of diffuse light between the two components supports the hypothesis of gravitational interaction and tidal disruption. Some bluer regions are visible, indicating the possibility of star formation triggered by the interaction. Overall, the system exhibits features consistent with an ongoing or recent merger event.
