The galaxy presents as an edge-on or near edge-on disk galaxy. There is a prominent central bulge exhibiting a yellowish-white hue, suggesting a significant population of older stars. The disk component appears elongated and relatively thin. The disk material is more diffuse and bluer than the central bulge. The disk shows faint structural features and appears relatively smooth, potentially with some spiral arms or dust lanes that cannot be definitively resolved at this resolution. The overall morphology implies a system with likely minimal ongoing major merger activity or strong tidal disturbances. There is a slight indication of truncation towards the end of the disk, the luminosity drops off relatively quickly.
