The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse halo fading into the background sky. The color gradient indicates an older stellar population with a yellowish hue dominating the central region. The outer regions appear slightly bluer, suggesting the presence of younger stars, though this feature is subtle. The galaxy is elongated, appearing cigar-shaped rather than perfectly spherical. There is no obvious sign of spiral arms, a bar, or significant dust lanes. The overall structure suggests a relatively evolved galaxy that is not undergoing any major mergers, though there might be some minor disturbances present within the galactic halo.
