The galaxy presents a distinct spiral morphology. The arms are tightly wound around a central bulge which is of moderate size. The disk appears largely undisturbed, exhibiting a fairly organized structure. There is evidence of multiple spiral arms. The spiral arms exhibit a tight winding pattern with distinct features. Color gradients across the galaxy suggest ongoing star formation within the arms, where regions appear bluer. The galactic disk is not edge-on. No strong bar feature is apparent. The central bulge displays a yellowish-white hue, indicative of an older stellar population.
