The galaxy presents as a spiral, observed at a near face-on orientation. It is characterized by a prominent central bulge, which appears yellow-white in color, suggesting an older stellar population. The spiral arms extend outwards from this central region, appearing somewhat fragmented and patchy, predominantly blue, with faint hints of reddish nebulae interspersed. Two distinct arms are easily visible, they are winding loosely. It does not appear to be undergoing a major merger but some minor disturbances are visible. There is no bar apparent. Overall, the galaxy exhibits moderate star formation, with an estimated effective radius of about 3 kpc.
