The galaxy appears to be a luminous elliptical type. Its morphology is dominated by a smooth, concentrated distribution of light, lacking any distinct spiral arms or a prominent disk structure. The color profile suggests a population of older stars, with a yellowish hue dominating the central region, indicating a potentially lower rate of recent star formation. The galaxy exhibits a generally round appearance, with only minimal deviation from a perfect circle. There is no visual evidence of ongoing major merger activity or significant tidal disturbances, although minor asymmetries could suggest a past interaction. The central region of the galaxy is significantly brighter than the outer regions, typical of galaxies with a high concentration of stars towards the center. The galaxy is relatively small and compact, especially for a larger elliptical galaxy.
