The galaxy presents an elongated, disk-like morphology, suggestive of a spiral or lenticular type viewed nearly edge-on. A prominent dust lane bisects the galaxy's central region, obscuring the light from stars within. The overall color appears to be bluer in the outer edges, indicating the presence of younger stellar populations. There is a brighter, more concentrated central bulge, potentially harboring an older stellar population. There are possibly two distinct bodies that exist in relation to each other, likely interacting or about to merge. The smaller, neighboring galaxy exhibits a smoother, less structured appearance. Overall, this galaxy displays characteristics indicative of a disk galaxy undergoing some form of interaction or disturbance. 
