The galaxy appears to be a spiral type, with a discernible disk structure. There is evidence of spiral arms, although they appear somewhat diffuse and patchy, with approximately half the community identifying them. The central bulge is prominent but is only considered to be moderate in size, with most community members in agreement. The disk component exhibits some asymmetry and fuzziness, potentially indicating ongoing or recent minor disturbances, but without any major interactions. A bar structure is possibly present, but it is indistinct. The overall colour of the galaxy is slightly bluish, suggesting a moderate level of star formation activity. The galaxy is relatively compact and appears to be at a relatively low redshift.
