The galaxy presents as a relatively compact, yet visibly structured object. It exhibits a disk-like morphology, though the spiral arms are not sharply defined. Instead, the galaxy shows flocculent spiral structure with patchy regions of star formation scattered throughout the disk, which is causing clumpy blue areas. The central bulge is moderately prominent and appears yellowish in color, possibly indicating an older stellar population. There is some indication of a minor disturbance in the galaxy's morphology, suggesting a potential interaction or merger event in its past.
