The galaxy presents as a spiral type, characterized by a prominent, albeit moderately sized, central bulge. The spiral arms are well-defined and extend outwards from the central region, exhibiting a clear two-armed structure. These arms display a medium winding, neither tightly wrapped nor widely dispersed. There is evidence of a bar-like structure extending through the center of the galaxy. The galaxy appears relatively undisturbed, showing no major signs of ongoing or recent merger activity. The disk is not edge-on, but clearly viewed from an angle.
