The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, exhibiting a high degree of roundness. The galaxy's light profile suggests minimal structural features such as spiral arms or a prominent disk. There are no obvious signs of tidal disturbances or ongoing major mergers. There is some indication of localized minor disturbances. The central region displays a relatively brighter, more concentrated luminosity suggesting a galactic bulge. Overall, the galaxy appears to be a mature system.
