The galaxy presents a generally smooth, elliptical morphology. Its light profile is centrally concentrated with a high degree of radial symmetry. The core exhibits a bright, yellowish hue indicative of an older stellar population. The isophotes appear quite regular with no obvious signs of strong tidal interactions or major disturbances. There may be some faint features suggesting a possible disk component, but the overall structure is dominated by a smooth, spheroidal shape. The faint outer regions have a reddish color, possibly indicating a population of cooler, older stars or dust obscuration. There is no clear evidence of active star formation visible in the image.
