The observed galaxy presents a distinct, elongated morphology. The structure appears as a flattened disk viewed at a high inclination, closely approaching edge-on. There is a noticeable central bulge that appears relatively smooth and concentrated. Moving outward from the core, the galaxy shows a fainter, more diffuse disk component. There is a hint of dust lane obscuration visible along the galactic plane, suggesting the presence of interstellar medium.

Overall, the galaxy's light profile is smooth and lacks significant patchiness or distinct spiral arm structures. It appears relatively isolated, with no immediately apparent tidal features or nearby interacting galaxies. The overall color is somewhat bluish indicating the presence of at least some young stars.
