The galaxy presents as a spiral, although the arms are tightly wound and somewhat difficult to fully resolve. The central bulge exhibits a moderate size relative to the overall disk. Within the bulge, the light is concentrated in the very central region. The disk appears to be dominated by the spiral arms. The color of the bulge appears more yellow/orange, suggesting an older stellar population. Blue hues are visible within the spiral arms, indicating regions of ongoing or recent star formation. There is some evidence of minor disturbances or asymmetry in the outer regions of the disk, potentially indicating a past or ongoing interaction with another galaxy. The galaxy is not observed edge-on. The spiral arm count is difficult to confidently determine with some arms being more diffuse and broken up. There is no strong evidence for a prominent bar structure in the central region of the galaxy.
