The galaxy presents as a relatively smooth, elliptical-like structure with a slight elongation. A concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population. The outer regions display a bluer tint, possibly indicating the presence of younger, hotter stars, although the smoothness dominates the overall morphology. There are no prominent spiral arms or bar structures visible. Minor disturbances cannot be ruled out, but do not dominate the appearance.
