The galaxy appears to be a smooth, elliptical type with a centrally concentrated bulge. It presents a generally rounded morphology, lacking any obvious spiral arm structures or significant asymmetries indicative of recent major mergers. There may be some minor disturbances in its shape, but it's primarily a regular spheroid structure. The light distribution is fairly even, with a gradual decrease in intensity from the core outwards. The color suggests a population of older stars, with a yellowish-red hue more dominant than a bluer, star-forming population. The galaxy exhibits a relatively compact appearance, indicating a high mass concentration within a small radius. The light from the galaxy is more luminous at the center than the edges.