The galaxy appears as a flattened, disk-like structure. A central bulge is visible, exhibiting a smooth texture. Evident are faint spiral arm features, primarily observed as subtle color variations throughout the disk. The disk's orientation presents an edge-on view, which obscures its central region. Faint dust lanes are suspected of traversing the disk, though obscured due to the image quality and edge-on presentation. There appears to be a lack of significant tidal disturbances or morphological irregularities, suggesting it is not undergoing a major merger event. A slight asymmetry is observable, which may indicate a minor interaction. The galaxy exhibits a color gradient, trending from bluer tones in the outer disk to redder tones in the central bulge. 
