The galaxy presents a clear spiral structure with noticeable arms extending from a central bulge. The arms are not tightly wound and appear somewhat flocculent, exhibiting patches of blue light suggestive of ongoing star formation within these regions. Dust lanes are faintly visible, tracing the inner edges of the spiral arms. The central bulge is prominent and has a yellowish hue, indicating an older stellar population. While the galaxy's overall shape appears relatively undisturbed, there are hints of asymmetry in the spiral arm structure. The disk of the galaxy dominates its appearance. No strong bar feature is apparent.
