The galaxy presents as a somewhat elliptical, though mostly rounded, structure with a smooth, diffuse appearance, concentrated in the center. The color profile suggests a dominant population of older stars, as indicated by the redder hue. No distinct spiral arms or features are readily apparent. The galaxy appears relatively undisturbed, showing no signs of recent major merger activity or significant tidal distortions. It displays a substantial spheroidal component. Star formation activity seems to be relatively low or currently suppressed within the observable portion of the galaxy.
