The galaxy presents a smooth, elliptical morphology. It appears largely featureless, with a high degree of central concentration of light. There is a discernible color gradient, with the core exhibiting a more yellowish-white hue, suggesting an older stellar population. The outer regions show a slightly bluer tint, which may indicate more recent star formation activity, albeit at a low rate. The galaxy exhibits a subtle disk like feature, and shows no obvious signs of ongoing mergers or major disturbances, although the structure seems slightly asymmetrical. 
