The galaxy presents as a luminous, elliptical form with a high degree of central concentration. Its light profile appears smooth and centrally condensed, exhibiting a radial falloff in surface brightness from the core to the outer regions. No distinct spiral arm structures are discernible. The core region is notably bright, with a gradual decrease in luminosity towards the outskirts. There is a subtle hint of dust absorption or patchy star formation regions on the periphery of the galaxy. The overall color suggests a population dominated by older stars, giving it a yellowish to reddish hue. Minor disturbances cannot be ruled out from the image.
