The galaxy presents as an elongated, cigar-shaped structure. A bright, centrally concentrated bulge dominates the visual appearance, exhibiting a yellowish-white hue. Surrounding the bulge, a fainter, bluish disk is discernible. This disk appears relatively smooth, lacking any pronounced spiral arm structures or significant dust lane features. The transition from the bulge to the disk seems gradual, with no sharp demarcation. There is a slight indication of ongoing star formation, suggested by the faint bluish tinge in the disk, and the overall shape suggests a system that may be either a lenticular or a tightly wound spiral galaxy viewed edge-on. There is no obvious indication of major mergers or strong tidal disturbances affecting the overall morphology, although a minor perturbation within the outer regions cannot be ruled out.
