The galaxy presents as a relatively smooth, concentrated elliptical system. A bright, yellowish central bulge dominates the morphology. The galaxy exhibits a diffuse, extended halo, fading into the background sky. The overall color suggests a population dominated by older stars. There is evidence of a slight, irregular feature in the halo region on one side, potentially indicating a minor gravitational interaction or past merger event. No significant dust lanes or spiral arm structures are apparent within the resolution of the image.
