The galaxy presents a largely smooth, elliptical morphology. The central region displays a high concentration of light, suggesting a significant stellar population. The light smoothly diminishes from the center outwards, forming a diffuse halo. There is some evidence of bluer colors in the outer regions compared to the central bulge, which appears more yellow. No distinct spiral arms or bar structures are visible. There appears to be only a very minor disturbance and no clear signs of an ongoing major merger. The galaxy's shape is generally in between round and elongated, appearing more oval.
