The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a strong, yellowish-orange hue, suggesting an older stellar population. The outer regions display a gradual decrease in surface brightness. There is a faint hint of a disk-like structure, however it is subtle and mainly featureless. No obvious spiral arms or dust lanes are detected. There are some indications of a very minor disturbance in its shape or structure.
