The galaxy presents a generally elliptical morphology, appearing largely featureless and smooth in texture. A concentrated central bulge is apparent, exhibiting a yellowish-white hue, potentially indicative of an older stellar population. The galaxy demonstrates a gradual decrease in surface brightness from its core outwards. A faint, diffuse halo surrounds the central region with a slight bluish tint. The absence of well-defined spiral arms or dust lanes suggests a relatively quiescent state of star formation. The shape appears close to circular with no noticeable elongations or distortions. No obvious signs of recent major mergers or tidal interactions are observed, although a slight asymmetry in the outer halo cannot be ruled out. The galaxy exhibits a regular, relaxed appearance.
