The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge region that transitions into a more diffuse, extended halo. The light distribution suggests a higher density of stars toward the center, gradually decreasing outwards. A slight elongation is apparent, leaning more towards an in-between circular shape. There are no immediately obvious signs of spiral arms or prominent dust lanes. No significant tidal disturbances or major merger activity are observed; however, there may be some evidence of a minor disturbance. Color gradients are subtle, with the central bulge appearing slightly yellower than the outer regions, potentially indicating a population of older stars in the core.
