The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. There is little indication of spiral arm structure or prominent dust lanes. The light distribution appears largely uniform across the galaxy’s body, with a gradual decrease in intensity from the core to the outer regions. Its roundness makes it appear almost circular. No signs of tidal tails or other obvious merger features are visible. There is only a slight hint of a disturbance in the central region. The galaxy's color is slightly yellow in the center, which could be indicative of an older stellar population. There is a high degree of smoothness and the galaxy is relatively undisturbed.
