The galaxy presents as a spiral galaxy with a notable disk structure. The spiral arms are prominent and tightly wound, suggesting a relatively ordered structure. The central bulge appears significant, but not overly dominant, indicating a moderate bulge-to-disk ratio. The galaxy does not appear to be perfectly face-on, showing a slight inclination, but not enough to classify it as edge-on. There is no visual evidence of a strong bar feature in its center. Indications of recent or ongoing star formation may be present within the spiral arms, as suggested by the subtle blue hues visible in some areas. No major disturbances or signs of a merger are apparent from this perspective, although minor disturbances cannot be ruled out based on the image alone.