The galaxy presents as a face-on spiral with a prominent central bulge. The bulge appears yellowish-white, suggesting an older stellar population. Two distinct spiral arms emanate from the bulge region, exhibiting a well-defined, although somewhat tightly wound, structure. These arms display clumpy regions of bluish light, indicative of active star formation within HII regions. The disk is relatively flat and has a high degree of axial symmetry. A strong bar feature appears to be present. Some disturbances are noted that could be due to a small merger.