The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. There appear to be two distinct, bright, and relatively round components, potentially representing the cores of the merging galaxies. The color of these components appears to be somewhat red, possibly indicating an older stellar population and subdued star formation within those regions. There is a faint, diffuse halo surrounding the bright components. The overall structure is quite complex and disturbed, indicating gravitational interactions are disrupting its original structure.
