The galaxy presents as a centrally concentrated, elliptical-like object with a smooth light distribution. The core exhibits a yellowish hue, suggesting a population of older stars. There are indications of a subtle gradient from the central region outwards, with the outer parts of the galaxy appearing slightly fainter and redder than the core. No distinct spiral arms or prominent dust lanes are visible. The overall morphology indicates the galaxy is likely in a relatively evolved state. There is no apparent interaction or merging events occurring. The galaxy appears fairly isolated, and the color suggests very low star formation.
