This galaxy presents a discernible disk structure oriented face-on relative to our line of sight. The spiral arms are readily apparent, exhibiting a tightly wound morphology. A central bulge is visible, occupying a moderate portion of the galaxy's overall spatial extent, but it is not the dominant structural component. There appears to be two tightly wound spiral arms. There are hints of ongoing star formation activity. The galaxy appears as an isolated system, showing no significant signs of major merger events or tidal disturbances. The galaxy presents a generally smooth appearance suggesting relatively low current star formation activity. There is a weak central bar.