The galaxy appears to be in the process of merging, or strongly interacting, with at least one other galaxy. It exhibits a disturbed morphology. The system is dominated by smooth components, rather than well-defined spiral arms or a prominent disk. The light profile is concentrated and relatively symmetrical, indicating a possible elliptical component. The galaxy displays a yellowish-red color, suggesting a population of older stars and relatively little ongoing star formation. There appears to be a possible tidal tail or bridge of material extending outwards, further supporting the interaction scenario. The overall shape appears moderately round.
