The galaxy appears as a flattened, disk-shaped structure, presented nearly edge-on from our perspective. A central bulge is visible, exhibiting a yellowish-white hue, suggesting a population of older, cooler stars. The disk is comprised of a bluer population, potentially indicating more recent star formation. There is evidence of dust lanes running along the plane of the disk, particularly obscuring the light from the central bulge. The edges of the disk are less well-defined, appearing somewhat diffuse. There is no evidence of a strong tidal interaction or major merger. A slight distortion to the disc is seen at one end, potentially due to a minor disturbance. The galaxy exhibits a relatively smooth morphology with some signs of a disk structure.
