The galaxy presents as a spiral, approximately face-on relative to our line of sight. Two distinct spiral arms are visible, exhibiting a moderate degree of winding. The central bulge appears prominent but not dominant, displaying a yellowish-white hue suggestive of an older stellar population. The disk component displays bluer regions indicative of active star formation. There is no visual evidence of a strong bar structure. Minor disturbances or possible early-stage merging activity are suggested. The galaxy is relatively symmetrical, with an ellipticity of around 0.84, or roughly 84% as wide as it is tall.
