The object under investigation presents as a late-type spiral galaxy observed edge-on. A prominent dust lane bisects the galaxy's major axis, indicating significant obscuration within the galactic plane. The central bulge appears relatively small and indistinct, exhibiting a smooth, diffuse profile with an elliptical shape, suggesting a later spectral type. The disk component is elongated and notably thin. There are a few concentrations of star formation within the disk, with a gradient of intensity toward the galactic center. The galaxy displays a high degree of flattening. No major disturbances or companions are apparent, suggesting a relatively isolated system.
