The galaxy presents a generally smooth, elliptical morphology. It appears as a centrally concentrated object with a diffuse halo. The core region is a bright, relatively unstructured area, possibly indicative of an older stellar population, while the outer regions exhibit a fading, slightly bluer hue, which might signify a small amount of recent star formation, though the overall star formation rate seems low. No distinct spiral arms or significant dust lanes are discernible. The galaxy exhibits no obvious signs of major mergers or tidal disturbances, suggesting a relatively quiescent evolutionary history. The galaxy is relatively compact.
