The galaxy presents as a spiral type, observed at a relatively face-on orientation. It exhibits a prominent central bulge, appearing bright and slightly elongated. Two distinct spiral arms emanate from the central region, tightly wound around the bulge. The arms are traced by regions of blue hues, suggestive of ongoing star formation. There is a strong bar-like structure present in the central region, which adds to the galaxies overall structure. The color distribution indicates a possible old stellar population, and areas of blue, indicative of some active star formation. No apparent signs of major mergers are seen. There are a few slight irregularities and disturbances in the galaxy, and the arm structure looks very clear.
