The galaxy presents a generally smooth, elliptical morphology. Its light profile is concentrated towards the center, displaying a bright, yellow-tinted core that gradually fades outwards. The overall shape is somewhat rounded, with only a slight elongation suggesting it is not perfectly spherical. There is no apparent evidence of strong spiral arms or a distinct disk structure. Subtle color variations are visible, hinting at differing stellar populations within the galaxy. A faint green hue can be seen around the edges, suggesting some star formation is taking place. While the overall structure appears relatively undisturbed, there may be minor irregularities present. These could potentially be signs of a past merger event, but further data would be needed to confirm this.
