The galaxy presents a largely smooth, elliptical morphology. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, indicative of an older stellar population. There is some evidence of a faint, disk-like structure surrounding the bulge. The arms lack prominent features and present with a blueish color, hinting at the presence of some ongoing star formation. The overall structure appears relatively undisturbed, without signs of major mergers or tidal disruptions. Some minor disturbances may be present. There is no visible dust lane.
