The galaxy presents a relatively smooth, elliptical morphology with a noticeable central bulge. The light distribution appears concentrated towards the center, indicating a higher density of stars in the nucleus. The galaxy exhibits a yellowish-orange hue, suggesting an older stellar population with fewer young, blue stars and more red giant stars. There is a slight elongation or deviation from perfect circularity. No distinct spiral arms or prominent dust lanes are visible, further supporting the classification as an elliptical galaxy. There are no obvious signs of major disturbances or ongoing mergers, though minor tidal features might be present at a level below the image resolution.
