The galaxy presents as a luminous, elliptical morphology with a smooth, centrally concentrated light distribution. The galaxy's color profile suggests a population of older stars, exhibiting a yellowish hue. There is no discernible spiral structure or prominent dust lanes visible. The galaxy appears relatively undisturbed, without significant tidal features or morphological irregularities indicative of recent major merger activity. The roundness of the galaxy is pronounced. Subtle color variations within the galaxy hint at varying stellar populations.
