This galaxy presents as a relatively small, late-type spiral galaxy seen edge-on. The galactic disk appears thin and elongated, exhibiting a notable dust lane that bisects the galaxy along its major axis. This obscuration suggests a significant presence of interstellar dust within the disk. The bulge is not very prominent and appears mostly rounded, and there does not appear to be a lot of star formation. There is no visual evidence of any tidal distortions or interactions with neighboring galaxies, suggesting that it is relatively undisturbed. It appears to be a relatively high mass galaxy given its magnitude.
