The observed galaxy presents as a grand design spiral galaxy, with a discernible disk component and tightly wound spiral arms. The color index indicates a potential higher presence of star formation regions in the arms relative to the bulge. The central bulge appears moderate in size, exhibiting a relatively smooth structure compared to the spiral arms. Two spiral arms are distinctly visible, with an overall loose winding pattern, suggesting a less sheared morphology. There is potential evidence of a weak bar structure spanning across the galactic center, though it is not distinctly prominent. Overall, the general form suggests a relatively unperturbed system, exhibiting no signs of on-going major merger events or significant tidal disruption. 
