The galaxy presents as a spiral galaxy, viewed nearly edge-on. The central bulge is relatively small and moderately bright, with a yellowish-white hue, suggesting an older stellar population. The disk component is extended, showing hints of spiral structure despite the nearly edge-on perspective. The spiral arms appear somewhat tightly wound near the bulge, becoming more diffuse towards the outer edges of the disk. There are some areas of blueish light in the disk, indicating regions of recent or ongoing star formation. The disk appears relatively smooth overall, lacking significant dust lanes or strong disturbances, although these may be difficult to discern at this orientation. No signs of a strong bar feature are apparent. There is no evident major ongoing merger event, though the possibility of minor tidal interactions cannot be ruled out.