The observed galaxy presents as a moderately inclined spiral galaxy with discernible, although somewhat diffuse, spiral arm structure. The arms appear flocculent in nature. The central bulge is small relative to the overall disk size. Some blue colors can be observed in the arms, which are indicative of recent star formation. There does not appear to be a strong central bar feature. Overall, the galaxy displays a morphology consistent with a late-type spiral, possibly of the Sc or Sd classification. There does not appear to be any evidence of ongoing major mergers, though there may be some minor asymmetries, possibly tidal disturbances, in the outer disk, but the quality of this image is difficult to make any definite claims.
