The galaxy presents as an edge-on spiral, characterized by a prominent central bulge that appears relatively smooth and concentrated. The disk is visibly elongated, displaying a high degree of inclination relative to our line of sight. The bulge exhibits a slightly boxy morphology, though the overall structure suggests a rounded shape. There is a noticeable absence of distinct spiral arm structures, which is expected for an edge-on galaxy. The color profile of the galaxy indicates a redder central region, likely attributable to an older stellar population within the bulge. The outer regions of the disk show subtle hints of bluer colors, possibly indicating the presence of younger stars, though this is not distinctly pronounced. No major disturbances or signs of a major merger event are apparent in the galactic structure, although very subtle signs of minor disturbance cannot be ruled out. The galaxy appears relatively isolated with a smooth overall morphology.
