This galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated, luminous region, appearing yellowish-white suggesting an older stellar population or dust obscuration. The light gradually decreases in intensity moving outward from the central bulge. Some faint bluish tinges are visible around the edges, possibly indicating areas of ongoing, though subdued, star formation. The galaxy's shape appears slightly elongated, perhaps deviating from a perfect sphere, with a hint of a disk-like structure. The overall appearance suggests a galaxy that may be in a relatively late stage of its evolution, with a modest star formation rate. There are no obvious signs of major mergers or significant tidal disturbances, though minor interactions cannot be ruled out.
