The galaxy presents as a relatively smooth, elliptical structure. There is a dominant central bulge with a high degree of circular symmetry. Evidence of a disk component is not readily apparent in the image. No strong indications of spiral arms or distinct features are observed. The galaxy exhibits a color gradient with a yellower-orange hue in the central region, suggesting an older stellar population. The outer regions appear slightly bluer, possibly indicating a younger stellar population or ongoing star formation, though the overall star formation rate is likely low. There are no signs of major mergers or significant tidal disturbances; any interactions appear minor, if present at all.
