This galaxy appears to be relatively compact with a bright, concentrated core. It exhibits a predominantly smooth morphology, although there are some noticeable features that suggest a degree of disturbance. The galaxy is primarily bluish-green in color, indicating the presence of younger, hotter stars and potentially active star formation regions. However, the smoothness fraction indicates a significant component of old stars or a lack of resolved features due to distance. A slight asymmetry or subtle distortion in the shape of the galaxy is evident, potentially related to past interactions or internal dynamics. There are hints of faint tidal features or diffuse extensions around the main body, but the image quality limits a definitive determination. 
