The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region that appears nearly spherical. The light profile indicates a high degree of central concentration, diminishing gradually outward. There is little evidence of spiral arms or a prominent disk structure. Color gradients suggest a population of older stars, with a yellowish hue dominating the core, transitioning to a redder color in the outer regions. No signs of significant dust lanes, tidal tails, or active galactic nucleus activity are apparent in this image. The object shows only a minor disturbance based on its morphology.