The galaxy appears to be an elliptical, with a high degree of central concentration. It has a generally smooth appearance, exhibiting little to no visible spiral arm structure. The galaxy's light profile gradually decreases in intensity from the center outward, without sharp edges or distinct features. The core of the galaxy presents a bright, yellowish-white coloration, indicative of an older stellar population dominating the center. There is a slight color gradient toward the outer regions. The central region is surrounded by a more diffuse, reddish halo. This suggests a population of older, redder stars in the outskirts, consistent with an aging elliptical galaxy. Overall, the morphology suggests a mature, relatively undisturbed system. There is some very minor distortion of the galaxy that could indicate a past merger.
