The galaxy appears as a relatively smooth, elliptical-like object. There's a concentrated central bulge, suggesting a high stellar density towards the core. The light profile appears diffuse with little sign of detailed structure such as spiral arms or distinct dust lanes. The color gradient shows a slightly bluer hue in the outer regions compared to the yellowish core, which could suggest younger star formation. No merging or major disturbances are easily apparent in this image, although a close examination with higher resolution data might reveal faint tidal features or signs of minor interactions. Overall, it appears to be a galaxy in a more advanced stage of its evolution with a smoother structure.
