The galaxy appears as an elliptical-shaped object with a smooth, diffuse light distribution. The core region exhibits a brighter, yellowish hue, suggesting a concentration of older stellar populations. Extending outwards from the core, the galaxy's luminosity gradually diminishes, forming a somewhat elongated halo. Subtle bluish tinges are observed at the furthest extents of the halo. The structure presents a degree of asymmetry, possibly hinting at a minor gravitational interaction. Overall, the galaxy appears relatively undisturbed with no obvious signs of ongoing major merger activity.
