The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be generally elliptical in nature but with moderate ellipticity, verging towards a rounder appearance. There is a hint of a more diffuse halo surrounding a brighter, more compact core region. Color gradients suggest some degree of color variation within the galaxy, potentially indicating differences in stellar population or dust content. The overall color is consistent with a galaxy dominated by older stellar populations, with a low star formation rate. No obvious spiral arm structures or strong tidal features are detected, supporting the smooth classification. No signs of an active galactic nucleus or intense starburst activity. Overall, it seems to be a relatively undisturbed galaxy of moderate mass.
