The galaxy presents a distinct disk-like morphology. The presence of spiral arms is strongly suggested, appearing somewhat tightly wound. A central bulge is discernible, appearing relatively moderate in size compared to the overall galactic structure. There is a hint of a bar-like structure spanning the central region of the galaxy. The disk is not edge-on, but oriented at an angle relative to our line of sight. Based on its color, the galaxy is potentially a site of ongoing star formation. The structure shows little evidence of any major disturbance or merger events. 
