The galaxy presents as a relatively smooth, elliptical form. The light distribution appears concentrated towards the center, indicating a prominent bulge. The color gradient suggests a population of older stars, with a yellowish hue dominating the visible spectrum. There is a subtle extension of light suggesting a disk in the galaxy, although no spiral arm structure is seen. No significant dust lanes or areas of active star formation are apparent. The overall morphology suggests a galaxy that has largely ceased active star formation and is dominated by an aging stellar population.
