The galaxy presents as a generally smooth, elliptical structure. Its core exhibits a concentrated, bright yellowish hue, indicative of an older stellar population. The galaxy appears somewhat oblong, with a slight elongation along its major axis, though not dramatically so. There is no discernible spiral arm structure. A faint, diffuse halo surrounds the core region, gradually fading into the background sky. No major disturbances or signs of ongoing mergers are apparent in its morphology. Overall, it appears to be a relatively undisturbed elliptical galaxy with a dominant older stellar population.
