This galaxy appears as a relatively smooth, elliptical-like structure. Its core region exhibits a concentrated, bright yellowish-white luminosity, which likely indicates an older stellar population. Surrounding the core, there's a diffuse halo that fades outwards. There may be a hint of a disk-like structure but it is very weak, indicating that the galaxy is more likely to be an elliptical galaxy, viewed nearly face-on. There are no apparent signs of ongoing major mergers or tidal disturbances, although there may be some weak evidence of minor perturbations in the outer halo region. Overall, the galaxy presents a regular and relatively undisturbed morphology.
