The galaxy presents as a centrally concentrated spheroid with a smooth light distribution. The color profile suggests a population of older stars, as evidenced by the redder hues in the outer regions transitioning to a bluer core. There are no apparent spiral arms or dust lanes. The galaxy appears relatively undisturbed, with no signs of tidal tails or other features indicative of recent merger activity. It exhibits a round morphology. Based on the color and smooth profile, this galaxy is likely an elliptical galaxy with moderate star formation activity.
