The galaxy presents a predominantly smooth morphology. The primary body exhibits a near-spherical shape, displaying high degree of central concentration. The color profile suggests an older stellar population, with a yellowish hue dominating the core region. There are no readily apparent spiral arms or a distinct disk structure. Subtle irregularities in the outer regions might indicate minor disturbances, possibly due to past interactions or accretion events. There is no evidence of recent major merger activity. Based on the color and morphology, this galaxy is likely a massive elliptical with little current star formation.
