The galaxy presents as a spiral type, exhibiting a relatively face-on orientation. A central bulge is discernible, appearing moderately prominent. Spiral arms are visible, displaying a well-defined structure and demonstrating a primarily tight winding pattern. There is a potential indication of a weak bar feature within the central region. The overall color profile suggests active star formation within the galactic disk. The morphology shows no clear signs of major mergers, though minor disturbances cannot be ruled out. The galaxy exhibits a generally smooth appearance with featured characteristics, but a relatively small smooth fraction. The galaxy's disk is clearly not edge-on. The size of the spiral arms cannot be properly assessed with the current image.
