The galaxy presents as a spiral type, viewed at an angle that is close to face-on. It exhibits a discernible disk structure. Within the disk, prominent spiral arms are apparent, displaying a relatively open and grand design. The arms appear somewhat patchy and flocculent, with regions of enhanced luminosity suggesting areas of active star formation. The nucleus appears relatively small and moderately bright. A possible bar structure seems to extend through the central region of the galaxy. There is a slight asymmetry in the distribution of light across the disk, possibly indicating a mild gravitational interaction or recent merger activity. The color gradient suggests a radial change in stellar populations, with bluer colors concentrated in the outer spiral arms, and redder colors more prominent towards the central bulge. Overall, this is a spiral galaxy with ongoing star formation within its arms, and a structure that indicates a history of interaction or merging events.
