The galaxy presents as a flattened, elongated structure, indicative of a disk galaxy viewed nearly edge-on. A central bulge is present, appearing somewhat diffuse and exhibiting a yellowish hue, likely indicating a population of older stars. The disk, extending outwards from the bulge, appears relatively smooth, with subtle color variations suggesting varying stellar populations or dust lane obscuration. The disk edges display a slightly bluer tint, potentially indicating regions of more recent star formation. No obvious signs of major mergers or tidal disturbances are apparent, although subtle asymmetries or minor disturbances may be present within the disk structure. Overall, the galaxy appears to be a relatively undisturbed disk system viewed at a high inclination angle.
