The object presents as an elongated galaxy, displaying a relatively smooth morphology. It exhibits a cigar-like shape, with its longest axis significantly exceeding its shortest. The light distribution appears fairly even and lacks obvious spiral arm structures or a prominent central bulge. The galaxy's color profile indicates relatively older stellar populations, which are consistent with low levels of on-going star formation activity. Minor disturbances may be present, but no signs of merging or major disturbances are observed. The object is not perfectly symmetrical, as one of its edges appears less smooth than the other. 
