The object appears to be a spiral galaxy, presenting with a face-on orientation. There is evidence of defined spiral arm structure, exhibiting a multi-arm morphology. The arms appear tightly wound around the central bulge. The central bulge is compact and displays a moderate size relative to the galactic disk. Star formation is likely ongoing within the spiral arms, suggested by the irregular texture and clumpy appearance with areas of increased blue color indicating younger stellar populations. There is a notable lack of a strong central bar structure. Based on the general morphology, the galaxy does not show clear indications of a major merger event, though there might be minor disturbances in the disk and arms which indicate past or ongoing interactions. The dust content appears moderate, based on the reddening observed towards the inner regions and along the spiral arms.
