This galaxy presents as a relatively smooth and featureless elliptical structure. The overall color profile indicates a general distribution of older stellar populations. There is a slightly brighter central region, likely representing a concentration of stars toward the galactic nucleus. The smooth morphology suggests a dynamically settled system, with minimal evidence of recent major mergers or significant tidal disturbances. The shape appears more in-between round and elongated. Weak star formation exists within the galaxy. 
