The galaxy presents as a face-on spiral, exhibiting a well-defined disk structure. Two prominent spiral arms emanate from a central bulge. The bulge appears moderate in size, exhibiting a yellowish-white color. A distinct bar structure is evident across the central region. The spiral arms display a medium winding, extending outwards. The arms show varying degrees of star formation, with some regions appearing bluer, indicating younger stellar populations. The overall morphology suggests the galaxy is not undergoing any major mergers or significant disturbances.
