The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its color profile indicates a relatively evolved stellar population, with a yellowish-white hue dominating the core region. There is a subtle color gradient, with the outer regions appearing slightly redder than the central bulge. This could suggest older stellar populations in the outer parts of the galaxy. No prominent spiral arm structures or significant dust lanes are discernible. The overall appearance suggests a lack of ongoing, major star formation activity. The object is nearly circular, with no obvious signs of tidal disturbances or recent merger events affecting its overall shape. It appears as a relatively undisturbed elliptical galaxy.
