The galaxy presents as a prominent, elongated, disk-shaped structure viewed nearly edge-on. A central bulge, characterized by a smooth, concentrated light distribution with a yellowish-orange hue, dominates the galaxy's core. Fainter, diffuse, bluish light extends outwards from the bulge, indicative of the galaxy's disk. No distinct spiral arm structures are apparent, likely due to the near edge-on orientation. The overall morphology suggests a relatively undisturbed system, showing minimal signs of ongoing or recent major merger activity. Faint dust lanes may be present along the midplane of the disk, however, these are difficult to resolve clearly at this resolution.
