The galaxy presents as a primarily smooth, centrally concentrated object. A slight disclike structure is suggested in the center with light bending slightly horizontally through the center. The system exhibits a blue hue, implying a significant population of young, hot stars and ongoing star formation. The morphology suggests a potentially disturbed system, possibly undergoing or having undergone a merger event, inferred by the non-uniform distribution of light within the galactic structure, and the merging fraction indicating a higher probability of being a merger.
