This galaxy appears to be a spiral galaxy viewed at an oblique angle, not quite edge-on but significantly tilted. The central bulge is moderately bright and not overly prominent, appearing somewhat blended with the disk. The disk exhibits a hazy or diffuse spiral structure. The spiral arms appear faint, especially in the outer regions. Patches of bluer light are visible within the arms, potentially indicative of active star formation regions or younger stellar populations. These regions are not as clearly defined or concentrated as one might expect to see in a grand design spiral, suggesting a flocculent or less structured arm morphology. There is no obvious bar structure.
