The galaxy appears to be relatively small and compact. The central region is bright and concentrated, possibly indicating a significant concentration of stars or an active galactic nucleus. There is a faint and diffuse halo surrounding the central region, suggesting a gradual decrease in stellar density with increasing distance from the center. The overall color profile suggests that the galaxy is bluer in its central region. There are possibly faint indications of minor disturbances or tidal features. Overall, the galaxy does not show any obvious signs of a merger. 
