The galaxy exhibits a disturbed morphology, indicating potential interactions or a recent merger event. The central region presents a bright, concentrated nucleus, surrounded by a more diffuse and less structured halo. One tail is observed, extending away from the central body of the galaxy. The system appears elongated, and the overall color is indicative of both evolved stellar populations and regions of active star formation. Patches of blue are indicative of star formation. Some regions appear disrupted. Overall, there is evidence that this galaxy may be interacting with another galaxy.