The galaxy presents as a spiral type. It exhibits a defined central bulge that appears elongated, suggesting the presence of a bar structure. Two prominent spiral arms emanate from the ends of the bar and are tightly wound around the central bulge. The overall color appears somewhat reddish, indicating a population of older stars and perhaps some dust obscuration. The disk is the dominant feature, with a moderate amount of star formation activity occurring within the spiral arms. There do not appear to be signs of any ongoing major merging events, although the overall structure seems slightly asymmetric, potentially indicating a minor interaction in the past.
