The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a yellowish-white color, suggesting a population of older stars. There is a slight elongation, but overall the galaxy presents a largely rounded appearance. Some minor disturbances are possibly present, but the overall structure suggests that it's more likely in the later stages of a merger, or has undergone a recent minor merger event. The lack of distinct spiral arms or significant dust lanes further supports this conclusion.
