The galaxy exhibits a clear disk structure with discernible spiral arms. The arms appear somewhat patchy, suggesting ongoing star formation. The central bulge is moderately prominent, indicating an intermediate morphological type, possibly between an Sb and Sc spiral. There is no evidence of a strong bar feature crossing the galactic center. The galaxy presents a relatively smooth appearance on the whole, although some minor irregularities and disturbances are visible, possibly indicative of past or ongoing interactions or mergers. The color profile suggests active star formation within the disk, with bluer regions tracing the spiral arms. The orientation of the galaxy is nearly face-on, allowing for a clear view of its spiral structure.
