The galaxy presents as a largely smooth, centrally concentrated object. Its morphology appears mostly elliptical, exhibiting a high degree of roundness with little discernible disk structure. The color profile suggests an older stellar population, with a central yellowish-white hue transitioning to a redder periphery. There are no obvious signs of ongoing major mergers or significant tidal disturbances, indicating a relatively quiescent evolutionary state. Faint blue tinges at the edges suggest pockets of star formation but at low levels. The galaxy's size appears moderate, consistent with a galaxy of substantial mass but not a giant elliptical.
