The galaxy presents as a relatively smooth, centralized concentration of light, exhibiting a high degree of symmetry. The central region displays a bright, concentrated luminosity, indicative of a possible galactic nucleus. The overall color appears yellowish-white. While a disk structure is not immediately apparent, subtle deviations in color and luminosity from the center outward suggest the presence of underlying features. A slight blue hue is present, especially at the lower and upper edges, potentially indicative of some star formation activity, although it is quite minimal. It is largely undisturbed, but it is difficult to say whether it is exhibiting minor disturbance, or merger activity.
