The galaxy appears to be a relatively smooth, elliptical-like structure with a moderately elongated shape. Its light is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is a subtle hint of bluer color towards one end, perhaps indicating a region of more active star formation, but the galaxy is generally characterized by a redder overall color, consistent with an older stellar population. There is a slight asymmetry or minor disturbance in the structure, potentially suggesting a past interaction or merger event.