The galaxy presents as a largely featureless, centrally concentrated object with a smooth overall appearance. The luminous core transitions into a diffuse halo, exhibiting a nearly circular morphology. The color gradient suggests older stellar populations are dominant. There is no apparent spiral arm structure or significant dust lane obscuration visible. Faint irregular features are scattered throughout the galaxy's outer halo. Based on color properties, the estimated star formation is comparatively low. There are no visible signs of ongoing or recent major merger activity.
