The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing bright yellow, suggesting an older stellar population. There is a gradual decrease in luminosity moving outwards from the center, with the outer regions appearing less defined and more diffuse. There is little visible structure, such as spiral arms or dust lanes, supporting the classification of a smooth, centrally concentrated galaxy. The galaxy appears largely undisturbed.
