The galaxy presents as a single, concentrated object with a smooth, elliptical morphology. It exhibits a central bulge that appears yellow-orange in color, suggesting a population of older stars. There is a lack of distinct spiral arms or prominent dust lanes, which supports the classification of the galaxy as elliptical. The light appears relatively uniform across the galaxy, with the highest concentration in the central bulge region, and a gradual decrease in luminosity towards the outer edges. There is no evidence of any significant ongoing mergers or tidal disturbances affecting the object's overall structure, and the galaxy's profile is relatively symmetric. The overall color suggests a galaxy with little current star formation.
