The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing elongated but without obvious spiral arm structures. The central bulge region is bright and has a yellow-white hue, potentially indicative of an older stellar population. Progressing outwards from the center, the galaxy displays a gradual decrease in luminosity. The outer regions are less defined, with a fuzzy appearance, and show a subtle transition to a bluish tinge. This hints at some recent star formation, though at a rate much lower than that of actively star-forming galaxies. The overall structure suggests a system that is not undergoing major mergers or tidal disruptions, although it is possible that it underwent minor merger events.
