The galaxy presents a lenticular morphology, displaying a prominent central bulge and a surrounding disk. The disk appears significantly inclined to our line of sight, presenting an almost edge-on profile. A distinct dust lane bisects the galaxy along its major axis, indicative of obscuration within the galactic plane. The bulge exhibits a smoother texture compared to the disk, suggesting an older stellar population. There appears to be some merging occurring as well, with disturbances. Overall, the galaxy seems to be experiencing suppressed star formation activity.