The galaxy appears to be a spiral galaxy, with evidence of a disk structure. The spiral arms exhibit a relatively tightly wound morphology, suggesting a classification along the lines of an Sa or Sb type galaxy. The overall color of the galaxy is bluish, hinting at the presence of younger, hotter stars and ongoing star formation, particularly in the spiral arms. A prominent central bulge is observed, although it does not appear to dominate the overall structure. The presence of a bar is difficult to definitively confirm based on the image alone, but there may be a subtle elongated feature across the central region. Indications of possible minor disturbances are present, such as asymmetry in the disk or irregularities in the spiral arm structure. Further investigation is needed to determine if these disturbances are due to interactions or mergers with other galaxies. The galaxy exhibits a relatively smooth appearance overall, but the spiral arms show some degree of clumpy structure.
