The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a relatively smooth light distribution without prominent spiral arms or significant dust lanes visible in this image. The galaxy core appears bright, suggesting a high density of stars, possibly indicating the presence of a supermassive black hole at the center. The overall color of the galaxy is bluish-white, which suggests a moderate population of relatively young, hot stars, possibly in the process of formation, but the smoothness of the galaxy suggests a more evolved system. The shape is mostly round, without any signs of major merger events. The periphery of the galaxy fades gradually, suggesting a halo of older stars extending beyond the main body. There might be some minor disturbances in the outer regions, potentially indicating a past or ongoing interaction with a smaller galaxy.
