The galaxy presents as a spiral type. It exhibits a prominent central bulge with a yellowish hue, suggesting an older stellar population within. The spiral arms are tightly wound and multiple, showing a distinct yet somewhat disorganized structure. Evidence of active star formation appears present within the arms, indicated by bluer regions. The galaxy is not seen edge-on, but with a slight inclination. There is a prominent bar-like structure bisecting the central bulge. There appears to be no major ongoing merger or significant tidal disturbance affecting the overall structure.
