The galaxy presents as an elongated, disk-shaped structure, viewed at a nearly edge-on orientation. The central bulge appears prominent and concentrated, exhibiting a yellowish-white hue, likely indicating an older stellar population. Moving outwards from the center, the disk displays a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. Dust lanes may be present along the galactic plane, though the resolution limits a detailed assessment. The outer regions of the disk fade gradually, lacking any distinct spiral arm structures, and show a flattened shape. Overall, the galaxy appears to be a relatively undisturbed system.
