The galaxy presents as a somewhat face-on spiral, exhibiting a central bulge that appears bright and elliptical. Diffuse spiral arms extend from the bulge region. The color gradient suggests older stellar populations concentrated within the bulge, transitioning to bluer hues further out, likely indicating ongoing star formation in the spiral arms. Dust lanes are faintly visible within the arms, obscuring some of the light from the stars. The overall morphology leans toward a grand design spiral structure, although the arms appear somewhat flocculent and not sharply defined. The galaxy is moderately inclined.
