The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth appearance. Its core exhibits a bright, yellowish-white hue, indicating a population of older stars. The luminosity gradually decreases outwards from the core, blending into a fainter halo of nebulous light. There's a subtle hint of bluer colors on the outer edges, potentially suggesting some degree of ongoing star formation. The overall morphology suggests a mature galaxy with minimal signs of recent major mergers or disturbances, yet may contain a disc feature. Its shape appears somewhat rounded but not perfectly circular.