The galaxy presents as a relatively smooth, elliptical structure. A concentrated central bulge dominates the light profile. The outer regions appear less concentrated and more diffuse. A slight elongation is discernible, moving toward a more disk-like appearance, though the overall structure remains primarily spheroidal. The central region exhibits a yellowish hue, which may indicate an older stellar population, while the outer regions show hints of bluer colors, possibly suggesting recent star formation activity, though at a relatively subdued rate. The overall structure appears undisturbed, without any significant tidal features or signs of a major merger event, although minor disturbances cannot be ruled out.
