This galaxy appears as a smooth, centrally concentrated object with a slightly elongated, elliptical morphology. The color gradient indicates a bulge with an older stellar population due to the presence of redder hues, which transitions outward into what appears to be a weak disk dominated by a younger population exhibiting bluer colors. There is little indication of significant dust lanes, spiral arms, or active star-forming regions. Overall, the galaxy seems relatively undisturbed, exhibiting no tidal features or signs of a recent major merger. The light profile gently decreases from the center to the outer edges, indicating a smooth distribution of stars.

