The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and centralized luminosity profile. The central region displays a bright, concentrated core with a yellow-white hue, suggesting a population of older stars. Moving outwards from the core, the color gradually shifts toward redder tones, indicating a continuation of the older stellar population. There are no distinct spiral arms or prominent dust lanes visible, reinforcing its classification as an elliptical galaxy. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. It exhibits a moderate degree of ellipticity, appearing more oval than perfectly spherical. Overall, it shows characteristics consistent with a relatively massive and evolved system.
