The observed galaxy presents as a spiral type, displaying a well-defined disk structure. The galaxy is not viewed edge-on; rather, it is presented at an angle revealing most of the disk. Two prominent spiral arms extend from the central bulge, exhibiting a relatively broad morphology and a medium pitch angle. These spiral arms are well-defined and extend across the majority of the galactic disk. A bar structure is suggested by the slightly elongated central bulge but is not a dominant feature. The central bulge appears moderately sized relative to the disk. The winding of the arms varies between tightly wound and loose, with regions appearing more tightly compressed while other regions appear looser. The color distribution suggests star formation is present within the spiral arms and potentially, although less prominently, in the central bulge. The overall structure shows no significant signs of recent major merger events or dramatic tidal disturbances, although minor disturbances cannot be ruled out.