This galaxy presents a distinct spiral structure. The arms are grand design, extending outward from a prominent central bulge. The arms are not tightly wound, and display a degree of patchiness, suggesting ongoing star formation regions. The central bulge appears relatively large, exhibiting a moderate presence. The overall color profile indicates a mix of stellar populations. The central regions appear yellower, indicative of older, redder stars, while the spiral arms exhibit bluer hues, suggestive of younger, hotter stars. There is a noticeable disk extending beyond the bulge and spiral arms. It does not show any signs of a major merger or extreme tidal disruption, but some minor disturbances or asymmetries are present. There is no strong bar structure visible, suggesting the galaxy is either unbarred or possesses only a weak bar.
