The galaxy exhibits a clear spiral morphology, with a prominent central bulge. Two main spiral arms emanate from the bulge, displaying a moderate winding. These arms appear somewhat flocculent rather than grand design. A central bar structure is subtly present. The bulge appears yellowish-orange, potentially indicating an older stellar population. Star formation regions, traced by blue-ish regions, are clearly visible in the outer arms. No strong evidence of major merging or tidal disturbances is immediately apparent. The galaxy is observed face-on.