The galaxy presents a predominantly smooth, elliptical morphology with a high degree of circularity in its overall shape. There is a concentrated central bulge exhibiting a bright, yellowish hue, suggesting an older stellar population. The outer regions show a gradual decrease in surface brightness, with a subtle fading towards the edges of the galaxy, and no discernible spiral arm structure. There are no signs of major disturbances or ongoing mergers in the image.
