The galaxy presents as a spiral galaxy with a relatively face-on orientation. Distinct spiral arm structures are visible, although somewhat diffuse. The arms appear flocculent, with regions of enhanced brightness suggestive of ongoing star formation. The central bulge is not particularly prominent and appears relatively small compared to the overall disk size. The overall color of the galaxy is bluish, consistent with ongoing star formation within the spiral arms, interspersed with regions of redder light, particularly in a few regions, which may indicate populations of older stars or dust obscuration. No strong bar structure is apparent. There are some suggestions of minor disturbances or asymmetries in the disk, potentially indicating past interactions, but no signs of a recent major merger. The galaxy is relatively isolated.
