This galaxy presents as a disk galaxy, viewed nearly edge-on from our perspective. A bulge is clearly visible, appearing bright and concentrated at the center. The bulge exhibits a yellowish hue, suggesting an older stellar population. Surrounding the bulge is a disk structure, which is less bright than the bulge. Dust lanes are not clearly resolved within the disk. The disk appears bluish near the edges. The shape of the galaxy is fairly smooth. There are no obvious signs of any major mergers, but some disturbances cannot be ruled out.
