The galaxy presents as a slightly inclined spiral, exhibiting a moderate bulge component relative to its overall disk size. The spiral arms appear somewhat flocculent and loosely wound, indicating a possible later-type classification. Dust lanes are faintly visible within the disk, particularly on the near side, contributing to the morphological features. The galaxy's color suggests a relatively evolved stellar population, with a noticeable redder hue. No signs of active galactic nuclei or intense star formation regions are immediately apparent. The overall structure suggests a relatively undisturbed and isolated system.
