The galaxy presents a moderately elliptical morphology. A concentration of older stars are seen throughout the central bulge region, giving it a yellowish-orange hue. The overall light distribution suggests a smooth profile, lacking prominent spiral arm structures or significant dust lanes. The galaxy appears to be undergoing a possible merging event, or tidal disruption with another galaxy, indicated by the dual nuclei, and overall disturbed morphology. The galaxy is relatively compact in size, with a high sersic index, suggesting this is an elliptical galaxy.