The observed galaxy exhibits a distinct spiral structure. Prominent spiral arms emanate from a central bulge region. The bulge shows a concentration of older stellar populations, indicated by its yellowish-white hue, with an estimated mass of 10^11 solar masses. The arms display a bluer color, indicative of ongoing star formation. The arms are well-defined, with a notable presence of three to four spiral arms. The winding of the arms appear to have a medium pitch angle, meaning they are not tightly wound nor completely unwound. There is no observable evidence of any significant tidal disturbances, which means any previous mergers may have fully completed. The galaxy is a relatively late-type spiral with a moderate bulge.
