The galaxy presents as a somewhat face-on spiral galaxy with a moderately bright central bulge. The arms are not sharply defined, appearing somewhat flocculent. The overall color index suggests a relatively old stellar population, though some bluer regions are present in the arms, indicative of ongoing star formation. There are no apparent signs of a major ongoing merger, though subtle disturbances are possible. The roundness indicates that it is not a barred spiral. The galaxy's apparent size is consistent with a moderately sized spiral galaxy at its redshift.
