The galaxy presents a generally smooth and elliptical morphology. The light is concentrated towards the center in a bright bulge, with a color index that appears redder than the outer regions. The radial profile suggests a gradual decrease in surface brightness away from the core, with a slight elongation. A faint disk-like structure can be observed extending beyond the central bulge, which indicates some level of rotational symmetry. The lack of distinct spiral arms or significant dust lanes suggest a relatively old stellar population dominating the light. There is little evidence of ongoing major mergers, though subtle disturbances might be present.
