The galaxy appears as a relatively smooth, elliptical-like structure, with a higher concentration of light towards the center. It exhibits a subtle color gradient, appearing slightly bluer towards its outer regions and redder in its core. There is a small indication of a faint disk. The galaxy’s overall form is neither perfectly spherical nor significantly elongated, but rather somewhere in between. There are no obvious signs of major disturbances or mergers and it presents as a relatively isolated system within the observed field.
