The galaxy appears as a singular, relatively homogenous, elliptical-like structure. It exhibits a smooth, diffuse light distribution. The galaxy's light profile is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is a subtle color gradient, with the core exhibiting a yellowish hue which gradually fades to a slightly redder tint further away from the center. No spiral arm structures or dust lanes are apparent. The overall structure seems undisturbed, with no visible signs of tidal tails, distortions, or recent major merger events. The galaxy appears to be isolated.
