The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish, possibly indicating an older stellar population. Moving outwards, the galaxy displays a gradual decrease in surface brightness. There is no strong evidence of spiral arms or significant dust lanes visible. The overall color profile suggests a galaxy that is somewhat evolved, with ongoing, but subdued, star formation activity. No strong signs of tidal disturbances or merging events are apparent. The galaxy’s shape is close to round, with only a slight hint of elongation along one axis. 
