The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish-white hue, indicating a likely concentration of older stellar populations. The outer regions show a gradual decrease in surface brightness, transitioning into a faint, more diffuse halo of bluish light. The overall color gradient suggests a potential decline in star formation activity from the center outwards. There is no apparent dust lane or spiral arm structure visible in this image, nor any indication of major mergers, although some minor disturbances cannot be ruled out at this resolution. The general round shape and smooth appearance are consistent with an elliptical classification.
