The galaxy presents as a spiral galaxy with a prominent disk structure. Evident spiral arms are visible, although somewhat diffuse and not tightly wound. The galaxy displays a relatively small bulge component, with a softly luminous central region. The overall color suggests ongoing star formation, with a bluer hue dominating the spiral arms. There may be some minor disturbances in the disk structure, but no signs of major merger events are immediately apparent. The galaxy appears to be relatively isolated.
