The galaxy exhibits a prominent disk structure. Evident spiral arms extend outwards from a central bulge, appearing somewhat tightly wound. The bulge itself appears to be of moderate size compared to the disk. The overall color suggests a relatively mixed stellar population, with some regions possibly exhibiting bluer hues indicative of more recent star formation. The disk shows some degree of disturbance, possibly hinting at minor interactions or internal processes. There is no clear indication of a strong bar feature. The galaxy appears relatively isolated within its immediate surrounding environment.
