The galaxy presents a distinct spiral morphology. Its structure is dominated by well-defined spiral arms that emanate from a moderately sized central bulge. The spiral arms appear tightly wound, exhibiting a somewhat flocculent structure with variations in luminosity along their lengths. The central bulge appears relatively bright and concentrated. There is an indication of a subtle bar-like feature running through the central region, though it is not overtly prominent. The disk component is observed nearly face-on, allowing for clear observation of the spiral arm structure. No significant signs of major tidal disturbances or ongoing mergers are readily apparent, although some subtle asymmetries within the spiral arms could suggest minor interactions or internal disturbances. The galaxy's overall color is slightly bluish, particularly along the spiral arms, hinting at ongoing star formation.