The galaxy appears as a lenticular system exhibiting a predominantly smooth morphology. It presents a flattened, disk-like structure viewed edge-on. The central bulge is moderately prominent, though its exact morphology is challenging to assess at this orientation. Evidence of a disk is limited to the overall flattened shape and subtle color variations, with some bluer regions interspersed. No pronounced spiral arm structures are visible. There may be signs of minor tidal disturbances. There is no indication of recent or ongoing major merger activity. Overall, the galaxy seems to be a relatively evolved and quiescent system.
