The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge, with a tightly wound structure. The arms display a noticeable presence of star formation activity, with some clumpy concentrations. The central bulge appears yellow, with lower levels of blue and red scattered throughout the galaxy. The disk appears to be the dominant feature, with a slight bar-like structure bisecting the bulge. No evidence of any interaction, major or minor, or a recent merger can be observed. The galaxy disk is tilted with respect to the observer's line of sight, showing a face-on orientation.