The galaxy presents as a largely smooth, elliptical structure. It exhibits a concentrated central bulge that appears bright and slightly blue-shifted. The light appears to fade gradually from the center outward, with a faint, diffuse halo extending beyond the primary body of the galaxy. There is no obvious dust lane or distinct spiral arm structure, suggesting it is either an elliptical galaxy or a spiral galaxy viewed face-on with minimal dust obscuration. No signs of active galactic nuclei activity are readily apparent, as the emission seems relatively uniform and consistent across the observed wavelengths. There is a slight elongation to the overall shape, which could indicate it is not perfectly spherical, tending more towards an oblate spheroid. There is no obvious evidence of strong tidal interactions or ongoing merging events with other galaxies.