The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an overall elliptical morphology, appearing nearly round in shape. The core region is bright and yellowish-white, indicative of an older stellar population. The outer regions display a gradual decrease in surface brightness, fading into a blueish hue. There is no obvious spiral structure or strong evidence of active star formation visible. Slight disturbances in the outer halo indicate a small chance of a minor merger. The overall appearance suggests a galaxy that is morphologically smooth with a dominant older stellar population.
