The galaxy exhibits a dual-component morphology. A dominant, centrally condensed spheroid with a smooth appearance is evident. This component shows a yellowish-orange color, suggesting an older stellar population with a reduced rate of ongoing star formation. A smaller, secondary component, also smooth in appearance, is located close to the primary component. The system displays signs of gravitational interaction, as the morphology hints at a possible ongoing merger or tidal disturbance. A significant fraction of light is concentrated within the inner regions, indicating a high central stellar density.
