The galaxy appears to be elliptical in shape, exhibiting a smooth, centralized light distribution. The core region displays a higher intensity of light, with a gradual decrease in luminosity extending outwards, suggesting a high concentration of stars towards the center. The galaxy's color is generally bluish-green, possibly indicating a population of younger, hotter stars, or active star formation. There is a subtle elongation. While no distinct spiral arms or disk-like structure are visible, subtle irregularities or minor disturbances may be present in the outer regions. Overall, the galaxy appears relatively undisturbed with no clear signs of a major merger event, although minor disturbances or faint tidal features might be present upon closer inspection.
