The galaxy presents as an elongated, disk-shaped system viewed nearly edge-on. It exhibits a prominent central bulge, which appears bright and concentrated, fading into a much more diffuse disk component. This disk shows mottled features, suggesting possible spiral arm structure, though the near edge-on orientation makes it difficult to definitively confirm. The color distribution indicates a yellow-white hue in the central bulge, becoming subtly bluer within the disk, which indicates that the bulge is composed of older stars, with the disk having populations of younger stars. This is supported by the star formation rates. The lack of strong dust lanes or obscuration suggests the galaxy may be relatively face-on with limited dust content, despite appearing edge-on. Furthermore, the galaxy exhibits a smooth overall morphology, lacking apparent signs of major mergers or tidal disturbances. The light appears to be smoothly distributed, indicating an evolved system.