The galaxy presents a generally smooth and concentrated morphology. It displays a roughly elliptical shape, although it leans toward being somewhat in-between round and elliptical. The core is noticeably bright, appearing a yellow-orange hue, suggesting an older stellar population. There is a very slight hint of a disk-like structure. There is no strong evidence of ongoing mergers or major disturbances. The outer regions of the galaxy fade into the background, showing a decrease in luminosity with increasing distance from the center.
