The galaxy presents as a relatively smooth, elliptical-like structure, although not perfectly spherical. It exhibits a moderate ellipticity, appearing somewhat elongated. The central region displays a brighter, more concentrated luminosity, fading gradually towards the outer edges. There is faint evidence of some minor internal disturbances or possibly faint spiral arms. The color appears generally uniform across the galaxy, suggesting a lack of significant dust lanes or distinct star-forming regions. The galaxy appears to be relatively isolated, with no obvious signs of major mergers or interactions. The galaxy's overall appearance suggests that star formation rate is low. The galaxy presents as a consistent red color.
