The galaxy presents a morphology consistent with a spiral galaxy, although the viewing angle obscures a clear face-on view. The central region appears bright and concentrated, indicating the presence of a prominent bulge. Faint and tightly wound spiral arms extend outwards from the central bulge, exhibiting a slightly flocculent structure, where the spiral arms are not continuous and well-defined. The arms show hints of bluer regions interspersed with older stellar populations. There is no evidence of a strong bar structure within the galaxy. There may be some irregular morphology or minor disturbance to the galaxy's overall structure, such as asymmetries or tidal tails. However, there is no clear indication of an ongoing major merging event.