The galaxy presents as a predominantly smooth, elliptical morphology with a high degree of central concentration. Its overall shape is largely round, showing minimal elongation or asymmetry. The core region is characterized by a bright, yellowish-white color, suggesting an older stellar population. A faint, diffuse halo surrounds the central region, exhibiting a gradual decrease in luminosity with increasing radial distance. No distinct spiral arm structures or prominent dust lanes are visible, further supporting the smooth classification. Subtle irregularities in the outer halo suggest the possibility of minor tidal interactions or past accretion events. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
