The object appears to be a spiral galaxy with a relatively high degree of symmetry. There is evidence of spiral arm structure, although the arms are somewhat diffuse and not tightly wound. There is a prominent central bulge, but it does not dominate the overall structure. The disk appears to be inclined at a moderate angle relative to our line of sight, not quite edge-on. There is little evidence of any significant ongoing merger activity or strong tidal disturbances. The overall color suggests a relatively high rate of recent or ongoing star formation.
