The galaxy presents as a single, relatively smooth, and centrally concentrated object. The overall shape appears approximately round. The core exhibits a yellowish hue, transitioning to a greenish color toward the outer regions. Faint, barely discernible irregularities suggest a possible minor disturbance, though the galaxy does not display any strong signs of an ongoing merger or significant tidal features. The light profile suggests an elliptical or lenticular morphology, with a substantial spheroidal component dominating the galaxy's structure. The color gradient from the center outwards indicates a potential decrease in stellar age and metallicity, or a change in dust content, toward the periphery.
