The galaxy exhibits a clear spiral structure with well-defined arms. A prominent central bulge is observed. The arms appear to be moderately wound and traced by regions of star formation. The disk appears to be observed at an angle from face-on. The galaxy shows some asymmetries in its disk structure, possibly indicating interactions or mergers. The presence of a bar may be present within the bulge but is difficult to determine given the quality of the image. There are clear color variations, suggesting differences in stellar populations across the galactic disk. The spiral arms seem to be of a more blue color than the bulge of the galaxy, suggesting differing stellar populations between the two.