The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge, characterized by a reddish hue, possibly indicative of an older stellar population. Moving outward from the core, the color transitions to a more yellow-greenish tone, suggesting a mixture of stellar populations with possibly some ongoing, though subdued, star formation. There is no discernible spiral arm structure. The overall morphology appears relatively undisturbed, lacking any prominent signs of tidal interactions or major mergers. The galaxy is somewhat rounded in its overall shape, not highly elongated or distorted. There may be minor disturbances present, but the smooth morphology dominates.
