The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms emanating from a central bulge. The arms appear relatively tightly wound, displaying flocculent structures and regions of active star formation, indicated by a bluer hue in these areas. The central bulge is prominent, appearing somewhat spherical and exhibiting a yellower colour, which suggests an older stellar population. There is a slight asymmetry to the overall galactic structure, potentially due to an interaction or internal processes. The galaxy displays a slight disc-like flattening.
