The galaxy presents a relatively smooth, elliptical morphology. Its central region appears bright and concentrated, exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy show a gradual decrease in luminosity, fading into the background. Faint, blueish wisps can be observed in the disk, hinting at possible star forming regions and dust. There may be some kind of disturbance in the gravitational field as the galaxy appears slightly asymmetrical. There may be a minor galaxy merger event taking place. The galaxy lacks a distinct spiral structure.
