The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears largely spheroidal, with a radial decrease in surface brightness. The color profile suggests a generally older stellar population, with a yellowish-white hue dominating the central regions. There's a subtle hint of bluer tones in the outer regions, possibly indicating the presence of some younger stars, or low levels of ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of tidal features or recent major mergers. No spiral arms or a well-defined disk are visible. The overall structure suggests a well-evolved system with minimal ongoing star formation within the field of view.
