This galaxy appears to be a spiral galaxy, viewed nearly edge-on from our perspective. It exhibits a flattened disk structure with a prominent central bulge that is relatively bright and appears somewhat rounded in projection. The disk of the galaxy shows evidence of dust lanes, appearing as darker regions silhouetted against the starlight, which are suggestive of ongoing or recent star formation activity within the disk. The color of the bulge is slightly redder than that of the outer disk, which might indicate an older stellar population dominating the bulge. The galaxy doesn't show signs of tidal disturbances or major mergers. It shows a relatively undisturbed morphology, appearing isolated. There is no clear bar structure apparent from the edge-on view.