The galaxy presents a mostly smooth, elliptical morphology. The core region exhibits a bright, concentrated luminosity, transitioning outward to a less intense, diffuse halo. There is a slight deviation from perfect circularity, appearing somewhat elongated. Subtle disturbances or features indicative of possible tidal interactions may be present, but are not overtly pronounced. A trace amount of blue color suggests a low-level of recent star formation in the outer regions, though the dominant color is indicative of an older stellar population.
