The galaxy appears to be undergoing a merger event. The structure exhibits a somewhat irregular morphology, with a dominant, smoother component and a secondary, more compact feature. The larger component shows a predominantly smooth light distribution, possibly indicative of an elliptical or lenticular galaxy. The smaller, more compact component displays a distinctly different color profile, appearing yellower, which may indicate a different stellar population or higher dust content. There is visible disturbance, indicating a gravitationally interacting system. The system's overall structure suggests a relatively advanced stage of merging. Tidal features appear weak or unresolved, which could be due to the distance of the system.
