The galaxy presents a disk-like morphology, viewed at an angle between face-on and edge-on. While the disk structure is evident, it appears somewhat diffused. Spiral arms are visible, exhibiting a two-armed structure that wraps moderately tightly around a central bulge. The bulge exhibits a moderate size relative to the overall galaxy. The spiral arms appear to be fairly continuous. A bar structure is potentially present, but the central region of the galaxy appears somewhat symmetric. The galaxy does not seem to be undergoing any major mergers or significant tidal disturbances, and the structure appears generally undisturbed.
