The galaxy presents a generally elliptical morphology. The central region exhibits a high surface brightness, appearing nearly uniform in color, with a yellowish-white hue suggestive of an older stellar population. The light tapers off gradually towards the outer regions of the galaxy. There is a subtle indication of a flattened disk-like structure, though the overall appearance is dominated by a smooth, bulge-like component. The outer regions appear fuzzier and less defined, possibly indicating a more diffuse distribution of stars or dust. No prominent spiral arms or distinct features are immediately apparent. There may be a very faint dust lane visible within the galaxy as well. The overall color profile suggests that the galaxy is relatively evolved, with ongoing but potentially modest levels of star formation.
