The galaxy presents as a single object undergoing what appears to be a significant merger event. The morphology is highly disturbed, with an amorphous central bulge that exhibits an extended tail. The light distribution is complex, displaying multiple, concentrated cores indicative of multiple interacting galactic nuclei. The system is not particularly well defined, and the tidal features are quite prominent, suggesting the merger is in a relatively advanced stage. The system exhibits a range of color variations across its structure, with slightly bluer regions indicating areas of recent or ongoing star formation, and redder regions which may indicate older stellar populations. The overall system's luminosity is high, considering its compact apparent size.
