The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The light profile appears centrally peaked, transitioning gradually outwards. A subtle color gradient is visible, with the core exhibiting a yellowish-orange hue which could imply an older stellar population. The outer regions present with a bluish tint, indicating the presence of some younger, hotter stars. No distinct spiral arms or significant dust lanes are discernible. There is no indication of ongoing major merging activity, though subtle irregularities in the outskirts may suggest minor tidal interactions or internal disturbances. The overall morphology suggests a galaxy undergoing passive evolution.
