The galaxy presents as a spiral, viewed at an oblique angle. A central bulge is prominent, displaying a relatively smooth and concentrated morphology. The spiral arms appear tightly wound around the central bulge, showing a distinct but somewhat patchy distribution of star formation.

The overall color gradient suggests the presence of a relatively older stellar population in the bulge, shifting towards bluer hues in the spiral arms indicative of ongoing or recent star formation. The disk exhibits a general symmetry. There is no obvious distortion suggesting ongoing major interactions or mergers with other galaxies. Dust lanes are not clearly visible.
