The galaxy presents a distinct spiral morphology. The spiral arms appear tightly wound around a bright, moderately sized central bulge. Coloration suggests active star formation regions are present, tracing along the spiral arms and concentrated in the central region. There is evidence of disturbance within the galaxy's structure, potentially indicating a recent or ongoing interaction or minor merger, with an asymmetry in its overall shape. A bar-like feature appears to be present although not distinctly, possibly weakly crossing through the central bulge, further influencing the spiral arm structure. The galaxy is not edge-on, presenting a face-on to slightly inclined view of the galactic disk.
