The galaxy presents as a relatively smooth, elliptical-like structure. A dominant central bulge is visible with a yellow-orange hue, which suggests an older stellar population. The outer regions exhibit a faint, diffuse halo with a slight green tint. No prominent spiral arms or dust lanes are discernible, and the overall form appears generally undisturbed. There is no strong evidence of active galactic nuclei or significant star forming regions in the image.
