The galaxy presents a prominent, centrally concentrated bulge that gradually diffuses into a more complex disk structure. The disk exhibits a distinct spiral pattern with several tightly wound arms extending from the central bulge. These arms are not very well defined; the winding is tightly packed near the bulge and appear to be a bit flocculent. The overall color of the disk is dominated by blue hues indicative of ongoing star formation, possibly related to the spiral arm structure. The bulge appears more yellow, suggesting an older stellar population. No apparent bar structure is visible. The galaxy appears relatively undisturbed with no signs of major mergers, although there are minor disturbances in the spiral structure.