This galaxy presents as a system undergoing a merger event. Two distinct galactic nuclei are visible, both exhibiting a yellowish hue suggestive of an older stellar population. A faint, extended tidal tail emanates from one of the nuclei, indicating gravitational interaction and disruption. The overall morphology of the system appears somewhat smooth, although the presence of tidal features hints at ongoing or recent interaction. The light from the two galactic cores is consistent with a substantial and relatively inactive galaxy. There is some evidence of possible distortion in the shape of the system, further supporting the classification as a merging or interacting galaxy pair. 
