The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright core with a yellowish hue, suggesting a significant population of older stars. Moving outwards from the core, the light gradually decreases in intensity. There is a subtle indication of a possible disk, but the overall morphology appears dominated by a smooth, spheroidal component. No prominent spiral arms or irregular features are discernible. The overall color suggests that this galaxy is a passively evolving system with a low rate of star formation. There is no apparent interaction or merger activity disturbing the overall symmetry of the galaxy.
