The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth overall morphology with a dominant spheroidal component. There is no clear presence of a disk or spiral arms. The color is primarily yellowish-orange, suggesting an older stellar population with a lower rate of ongoing star formation. The light is centrally condensed, which likely means that most of the stars reside in the center of the galaxy. Some light extends into the outskirts of the galaxy, suggesting a halo. The galaxy is quite large. It appears largely undisturbed, showing no clear signs of recent major merging activity, though minor disturbances cannot be ruled out.
