The galaxy presents as a spiral type, exhibiting a well-defined disk structure with prominent spiral arms. These arms display a relatively moderate winding. They appear to originate from a central bulge. The bulge exhibits a noticeable contribution to the galaxy's overall luminosity. The disk shows a mottled texture with a distribution of star-forming regions along the arms, evidenced by the irregular brightness. No major disturbances are visible, however some minor disturbance cannot be ruled out given the image quality. The orientation suggests a face-on view. The color profile implies a diverse stellar population, with a relatively high mass.
