The galaxy presents as a relatively smooth, elliptical structure. There is a concentrated central bulge that fades outwards to a more diffuse halo. The color is generally yellowish-white, suggesting an older stellar population and diminished star formation activity. The lack of distinct spiral arms or prominent dust lanes supports classification as an elliptical galaxy. There is a subtle elongation, deviating slightly from a perfectly circular profile. No signs of recent or ongoing major mergers are apparent, and the morphology appears undisturbed.
