The object appears to be a galaxy undergoing a significant merger event. The morphology is highly disturbed, exhibiting two distinct, bright central concentrations of light, suggestive of two galactic nuclei in close proximity. There is a faint, diffuse halo of light extending outwards, indicating potential tidal interactions and disrupted stellar populations. The primary color of the galaxy is yellowish-red, implying an older stellar population with possibly ongoing, but not dominant, star formation activity. A disk is not clearly discernible, but it is possible that one exists and is being disrupted by the merger. The galaxy appears fairly compact, though with possible tidal features distorted due to gravitational interactions. The morphology suggests a late-stage merger.
