The galaxy presents as a prominent, elongated structure, viewed nearly edge-on. A central bulge region appears with a yellowish-orange hue, suggesting an older stellar population, potentially dominated by evolved stars. Extending outwards from the bulge, a fainter, bluish disk is visible, indicating the presence of younger, hotter stars and ongoing star formation. The disk appears relatively smooth, though some subtle irregularities are visible. The galaxy lacks any obvious signs of a major ongoing merger. The orientation of the galaxy allows for a clear view of its overall shape and structural components. The galaxy displays a moderate degree of concentration, with the light centrally peaked towards the bulge.