The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. It possesses a nearly circular morphology, with an absence of any significant disk-like features or spiral arms. There is a gradual decrease in luminosity from the central core outwards, indicating a smooth stellar distribution. The galaxy exhibits a yellowish-white hue, suggesting a dominant population of older stars, and a low rate of current star formation activity. No apparent signs of tidal disturbances or ongoing mergers are detected in this image, indicating it is a relatively undisturbed system.
