The galaxy presents as a relatively smooth, elliptical-like object. Its central region exhibits a high surface brightness with a yellowish hue, suggesting a population of older stars. The light profile appears to fade gradually outwards from the center, transitioning into a fainter, more diffuse halo. The overall shape deviates slightly from perfectly round, with a subtle elongation implying a possible disc component or triaxial structure. There are no prominent spiral arms or significant dust lanes visible. Overall, the morphology suggests a relatively evolved system with minimal ongoing star formation and no indications of major merger activity.
