The object appears to be a spiral galaxy with a moderately inclined disk. Spiral arms are clearly visible, displaying a somewhat flocculent structure. Two dominant arms are prominent, and are wound moderately tightly. There appears to be a small bulge at the center, although the arms extend reasonably close to the nucleus. There appears to be areas of active star formation taking place in some of the arms, judging by the slightly bluer light concentrated within. The galaxy itself seems relatively isolated, without any clear signs of major interactions or disturbances. There may be a weak bar structure present, extending across the central bulge. 
