The galaxy presents an elliptical morphology with a smooth, concentrated light profile, suggesting an early-type classification. The light is more concentrated toward the center of the galaxy. The galaxy displays a subtle color gradient, transitioning from a more yellow/white core to a slightly bluer outer region. Overall, the galaxy exhibits a cohesive structure with no discernible spiral arm features or obvious signs of recent major merger events. However, subtle disturbances in its outer regions may hint at minor interactions in its past or ongoing low-level accretion.
