This galaxy exhibits a primarily smooth, elliptical morphology. It presents a luminous core region which gradually diffuses outwards into a less defined halo. The color profile suggests an older stellar population, with a yellowish hue dominating the central regions, potentially indicative of minimal ongoing star formation and a prevalence of evolved stars. Slight irregularities in the outer halo might suggest minor gravitational interactions, although no obvious merging events are apparent. The overall shape is somewhat elongated, leaning towards an intermediate ellipticity rather than being perfectly spherical. The galaxy appears relatively undisturbed.
