The galaxy presents as a luminous, elliptical-like structure with a smooth, concentrated central bulge. A slight elongation in the galaxy's shape suggests it is not perfectly spherical. The color gradient indicates an aging stellar population, with a yellowish hue dominating the central regions, implying older, cooler stars. A small, redder and relatively compact region is observed to the side, potentially an area of ongoing star formation or a background object not associated with the galaxy itself. The overall smooth appearance of the galaxy suggests it is a relatively undisturbed system, showing no significant signs of recent major merger events.
