The galaxy presents as a face-on spiral, with a prominent central bulge and a disk characterized by distinct spiral arms. The bulge exhibits a yellow-orange hue, suggesting an older stellar population. The spiral arms appear somewhat tightly wound, displaying a mix of blue and white regions indicative of ongoing star formation, along with dust lanes that trace the spiral structure. The arms appear somewhat fragmented and not as well defined. There is no obvious bar feature, but a disturbance in the disk or very weak bar feature cannot be ruled out. The galaxy shows no obvious signs of a major merger or tidal disruption, however, a minor disturbance is possible. The galaxy seems to have an intermediate amount of dust attenuation as indicated by color gradients across the image.
