This galaxy presents as a merging system. There are two distinct nuclei visible, indicating a probable ongoing or recent merger event. The overall color is yellowish-white, suggesting a significant population of older stars. There is a lack of distinct spiral arm structure, and there are significant disturbances and asymmetry in the galactic structure, likely due to gravitational interactions during the merger. The morphology is generally round, but the shape is heavily distorted due to the merger. 
