The galaxy presents a largely smooth, elliptical morphology. The color profile indicates a concentration of older stellar populations, with a slight bluer hue in the central region, suggesting some ongoing, albeit subdued, star formation activity. The galaxy appears largely undisturbed, without any significant signs of tidal interactions or major mergers. It exhibits a relatively concentrated light profile, indicative of a high degree of spherical symmetry, with the majority of light concentrated in its core. There are no visible spiral arms or prominent dust lanes. It is not perfectly spherical, but has a shape that lies somewhere between an elliptical and a spiral galaxy. 
