The galaxy presents as a primarily smooth, elliptical structure. There is a bright central bulge, yellowish in color, suggesting a concentration of older stellar populations. Surrounding the core is a more diffuse halo with a bluish tint, potentially indicating the presence of younger, hotter stars and ongoing star formation, albeit at a relatively low rate. The overall shape is somewhat elongated, deviating slightly from a perfect sphere, but lacking any strong indications of spiral arms or a well-defined disk. There are no obvious signs of major mergers or significant tidal disturbances in its immediate vicinity, with just a subtle asymmetry in its outer regions.