The galaxy appears to be a luminous elliptical, exhibiting a smooth, centrally concentrated morphology. The core region is a bright, yellowish-white, suggesting an older stellar population. The galaxy is elongated, appearing as a flattened spheroid rather than a perfect sphere. There may be a slight, subtle dust lane or other irregularity, though this is unclear due to image resolution and a lack of distinct features. The outskirts of the galaxy gradually fade into the background, indicating a decreasing stellar density with increasing radial distance. Overall, the galaxy seems undisturbed, showing no obvious signs of a recent major merger event.
