The galaxy presents as a spiral galaxy with a moderately sized bulge. The spiral arms appear fairly distinct, exhibiting a two-armed structure that is wound relatively tightly around the central bulge. There is a suggestion of a bar feature crossing the central bulge, with moderate strength. The primary plane of the galactic disk is oriented between edge-on and face-on relative to our line of sight, with the spiral arms largely visible. A small degree of minor disturbance is apparent, which suggests the galaxy may be involved in a minor merging event. The galaxy exhibits varying regions of color and luminosity, which suggest active star formation. The disk is primarily bluer, while the bulge appears more yellow and old. 
