The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. The arms appear somewhat flocculent, with a mix of tightly and moderately wound morphologies. The central bulge appears moderate in size relative to the disk, with a bright core. There is evidence of a stellar bar structure spanning the central region. The disk shows some evidence of ongoing star formation activity, indicated by the bluer color. There are some indications of potential minor disturbances in the galaxy's overall structure. The galaxy is not observed edge-on.
