The galaxy presents as a primarily smooth structure with a hint of disk-like morphology. It appears elongated, with an approximate cigar-shaped profile. The central region is slightly brighter and more concentrated, transitioning to a fainter, diffuse halo or disk. The galaxy's color suggests ongoing, though not extremely vigorous, star formation activity, exhibiting bluer hues. There are indications of minor disturbances or asymmetries, possibly suggesting past interactions or mergers. 
