The galaxy presents as a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology with a roughly round appearance, showing minimal discernible disk structure or spiral arms. The galaxy's light profile suggests a single, dominant component with a gradual decrease in luminosity moving outward from the core. The color gradient transitions from a bright yellowish-white core region to a slightly redder halo. There is no evidence of significant ongoing mergers or tidal disturbances in the immediate vicinity.
