The galaxy presents a largely smooth and centrally concentrated light distribution. Its morphology appears generally elliptical, with a high degree of circularity. The core of the galaxy exhibits a bright, yellowish-orange hue, suggesting an older stellar population. This color profile fades outward, transitioning to a more diffuse and reddish outer halo. No distinct spiral arm structures or prominent dust lanes are discernible. There may be some minor disturbances in the shape. The overall appearance suggests a system with relatively low ongoing star formation.
