The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicating a population of older stars. Diffuse light extends outward from the central region, fading gradually into the background. There is an absence of distinct spiral arms or prominent dust lanes. The overall structure appears smooth and relatively undisturbed. Based on the color profile, star formation may be minimal, but not entirely absent. There's no visually significant tidal features to suggest a recent major merger event, although minor disturbances cannot be ruled out.
