The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that is yellowish in color, possibly indicating an older stellar population. Moving outwards from the center, the galaxy displays a gradual decrease in surface brightness, transitioning to a bluish hue. This color gradient may suggest ongoing star formation within the outer regions. The overall morphology suggests a relaxed system without any significant tidal disturbances or evidence of recent major mergers. The galaxy displays a somewhat regular, round shape. There may be some minor asymmetries within the outer disk. 
