The galaxy presents as a diffuse, elliptical-like object with a smooth, centrally concentrated light profile. The core exhibits a bright, yellowish-orange hue, indicative of an older stellar population or dust obscuration. Moving outward from the core, the light gradually fades into a more greenish and less distinct halo. While the main body appears relatively undisturbed, subtle color variations and asymmetries in the outer regions suggest possible minor interactions or past merger events. The overall structure lacks the distinct spiral arm features or a prominent disk, reinforcing its classification as an elliptical galaxy. The slight elongation suggests it could be transitioning from a more spherical to a somewhat cigar-shaped form, although the deviation is minimal. The smooth light distribution implies a relatively stable and evolved system with ongoing, albeit subdued, star formation activity.
