The galaxy presents a largely smooth, centrally concentrated morphology. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions display a bluer color, suggesting the presence of younger, hotter stars and possibly ongoing star formation. The galaxy appears relatively undisturbed, without any obvious signs of a major merger event or significant tidal distortions. There might be the faintest hint of a disk structure, but is hard to discern. Overall, the galaxy has an elliptical appearance with a relatively high degree of central concentration.
