The galaxy presents as a disk galaxy, observed at a near face-on orientation. The spiral arms are not sharply defined, suggesting a flocculent or grand design spiral structure with low contrast. A central bulge is discernible, appearing moderately sized relative to the overall disk. There is evidence of a bar structure traversing the bulge along the galaxy’s major axis. Star formation appears to be ongoing, as evidenced by the blue color of the disk, though the rate appears to be relatively low. No signs of major mergers are seen, although minor disturbances in the disk's structure may be present. 
