The galaxy presents as a somewhat elliptical, centrally concentrated object. The core region exhibits a yellowish-white hue, potentially indicating an older stellar population. The outer regions display a bluer tinge, which could be indicative of ongoing or recent star formation activity. There is a high degree of smoothness in the galaxy's overall structure, with no prominent spiral arms or distinct features that point to recent major merger events. A slight elongation is observed, though the galaxy is generally considered round rather than highly elongated. A hint of disturbance or asymmetry can be observed, but is minimal.
