The galaxy appears to be a spiral galaxy, viewed at a moderate inclination. It exhibits a central bulge that appears relatively smooth and somewhat elongated. Surrounding the bulge is a disk, showing evidence of spiral arm structure, though the arms are not tightly wound and appear somewhat flocculent. The disk exhibits a blueish hue, particularly in the outer regions, suggesting ongoing star formation. A reddish color is visible in the inner regions and bulge. The galaxy does not display any obvious signs of major mergers or significant tidal disturbances. The overall morphology suggests a galaxy undergoing moderate star formation activity within its disk.
