The galaxy presents as a centrally concentrated object, with a relatively smooth overall appearance. It appears elliptical in shape, exhibiting a high degree of roundness. The core region presents a yellowish hue, potentially indicating an older stellar population, while the outer regions are tinged with a bluish color, suggestive of a younger stellar population and possibly ongoing star formation. No spiral arm structures or significant dust lanes are discernible in the image. There are no obvious signs of a major merger or tidal disturbances. The overall morphology suggests an early-type galaxy, transitioning from disk-dominated to spheroidal, with possible low-level star formation occurring in the outer regions.
