The galaxy presents as a disturbed system, possibly undergoing a merger event. There appear to be multiple distinct luminous regions, with the largest and most prominent showing a bluish hue suggesting recent star formation. The overall shape is irregular, without a well-defined spiral or elliptical structure. The light distribution indicates that the galaxy is likely in a dynamic state, with ongoing gravitational interactions influencing its morphology. Patches of diffuse light may indicate tidal features and disrupted material indicative of such a merger event.

