The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, suggesting an older stellar population. The isophotes become slightly more reddish moving outward from the core, indicating a possible change in stellar population or dust content. No prominent spiral arms or disk structures are discernible within the available resolution. There are no signs of strong tidal features or morphological disturbances suggestive of a recent major merger event. The galaxy appears relatively undisturbed, potentially representing an evolved system.