This galaxy presents as an edge-on spiral galaxy, characterized by a relatively smooth, elongated structure. The central bulge appears prominent and elongated, with a slight boxy shape, exhibiting a concentration of older stars that contribute to its yellowish-orange hue. The disk is observed nearly edge-on, with limited visible dust lanes along the central plane, but there is evidence of some obscured regions. The overall form indicates minimal signs of recent major mergers or significant tidal disturbances, with the spiral arms appearing tightly wound and relatively undisturbed. Star formation is likely ongoing within the disk, but it is at a moderate rate, as evidenced by the relatively consistent color across the galactic plane.
