The galaxy presents as a spiral, viewed at an oblique angle. It possesses a notable disk structure exhibiting defined spiral arms. The arms appear tightly wound near the central bulge, with a hint of flocculent structure, and are resolvable as they extend outwards. There may be multiple arms, although the exact number is difficult to determine from this image. The central bulge appears relatively small and not overly prominent, exhibiting a smooth, concentrated light profile. Color gradients suggest ongoing star formation, particularly concentrated along the spiral arms as evidenced by blue hues, while the central region appears yellower in color, indicating an older stellar population. There is no indication of any major merging events, although there may be some minor disturbances in the outer disk. The overall morphology is indicative of a late-type spiral galaxy with a moderate redshift.