The galaxy presents a largely smooth morphology. It exhibits a centrally concentrated luminosity profile, suggesting a dominant bulge component. The overall shape appears nearly circular. The central region presents a yellowish color, possibly indicating an older stellar population, while the outer regions appear somewhat bluer. There are no obvious spiral arm structures visible, and no clear signs of ongoing major merger activity, though minor disturbances cannot be ruled out. The galaxy's estimated size suggests that it is a relatively large galaxy. 
