The galaxy presents a distinct spiral morphology. The disk is oriented somewhat face-on, allowing a good view of its spiral arm structure. The arms appear flocculent and somewhat tightly wound. Evidence suggests two dominant spiral arms, although some fainter arm segments may exist. The central bulge is moderately sized and appears yellowish, which may indicate a population of older stars. There's no clear bar structure visible. Patches of blue light along the spiral arms are suggestive of ongoing star formation. The galaxy shows signs of minor disturbances and the possibility of minor interaction with another galaxy.
