The galaxy presents as a spiral type, viewed from a nearly face-on orientation. Two prominent spiral arms emanate from the central region and extend outwards. The arms exhibit a loosely wound morphology. Evidence of star formation is apparent within the spiral arms, indicated by a mottled texture and subtle variations in color. The central bulge is moderately sized, gradually blending into the surrounding disk. A weak bar structure is present across the center. No signs of major mergers or significant disturbances are evident.