The galaxy presents as a relatively large spiral with a moderate bulge. It has two distinct spiral arms. The spiral arms appear somewhat tightly wound. The central bulge exhibits a yellowish hue, indicating a population of older stars. The disk of the galaxy shows a bluer tint, suggesting the presence of younger stars and ongoing star formation. A faint bar structure appears to extend through the center of the galaxy. There is a slight indication of a minor disturbance in the disk, potentially due to a recent interaction or merger. The overall morphology suggests an actively evolving system.
