The galaxy presents as an elliptical morphology, exhibiting a smooth and centralized light distribution. The object's color profile indicates a concentration of older stellar populations, with a yellow-orange hue dominating the central region and gradually fading towards the outer edges. No distinct spiral arms or dust lanes are discernible in the image, consistent with an early-type galaxy classification. The galaxy exhibits a high degree of roundness, with an axis ratio close to unity, appearing nearly circular in projection. There is no obvious evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure.
