The galaxy appears to be a relatively smooth, centrally concentrated elliptical system. Its overall color is indicative of an older stellar population, displaying a yellowish-orange hue. There is a lack of distinct spiral arm structures or prominent dust lanes. The galaxy presents a somewhat spherical shape, with a high degree of central light concentration. No obvious signs of active galactic nuclei or ongoing major mergers are discernible. The absence of distinct features suggests that star formation activity is relatively quiescent within this galaxy. Faint extensions or a diffuse halo may be present, but the image quality limits the ability to determine fine details.