The galaxy presents as a relatively smooth, elliptical structure. It exhibits a discernible color gradient, transitioning from a redder core region to a greenish-yellow hue in the outer portions. The light distribution suggests a moderate degree of central concentration. While the overall form is elliptical, there is a slight elongation, indicating it is not perfectly spherical, or perhaps there is a hint of a disk. There is no clear evidence of spiral arms or significant dust lanes. Its color suggests the presence of both older stellar populations in the core and perhaps younger stars in its outer regions. There is no evidence of major mergers or disturbances in the image, the galaxy appears relatively undisturbed.
