The galaxy presents as a relatively smooth, centrally concentrated object with a subtly elliptical morphology. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue. There is no prominent disk structure visible, and the galaxy appears largely undisturbed, showing no signs of significant tidal interactions or recent major mergers. A faint hint of extended halo is present. Based on its morphology and color, this galaxy may have a low rate of star formation.
