The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a generally smooth morphology, with no readily apparent spiral arms or distinct disk features. The galaxy's color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region, potentially indicating a lack of significant ongoing star formation. The light intensity peaks sharply at the center, decreasing gradually toward the periphery, forming a somewhat rounded shape. There is a possible slight disturbance visible on one side. This morphology is broadly consistent with an early-type galaxy, potentially a massive elliptical galaxy that has undergone significant evolutionary processing.
