The galaxy presents as a centrally concentrated elliptical system. The overall color profile indicates a greater abundance of older stellar populations, manifesting as a yellowish hue. The galaxy exhibits a smooth morphology, devoid of any prominent spiral arm structures or significant dust lane obscuration. There is a notable lack of irregular features suggesting relative dynamical stability and the absence of major ongoing merger events. The isophotes appear fairly regular and elliptical, with a high degree of axis symmetry, indicating a relatively relaxed and well-mixed stellar distribution. The galaxy appears nearly face-on. There may be little to no active star formation observed in this image.
