The galaxy presents as a structured object with a notable spiral morphology. The arms appear somewhat flocculent and exhibit a complex structure. A central bulge is discernible, though not exceptionally prominent, and exhibits a fairly smooth texture. There is a clear difference in color and brightness between the bulge and the arms, suggesting differing stellar populations or dust content. The spiral arms seem to be partially resolved into individual star-forming regions. There is evidence of asymmetry, possibly indicative of an interaction or an internal instability. The overall color suggests a galaxy with both older stellar populations and ongoing star formation.
