This galaxy presents as a spiral structure, observed at a considerable inclination relative to our line of sight. Distinct spiral arms are discernible, though they are not tightly wound. Two prominent spiral arms appear to be dominant. The arms exhibit a somewhat flocculent morphology, with regions of enhanced brightness potentially indicating active star formation. A central bulge is present, appearing neither particularly dominant nor absent, showing an intermediate size. There is no obvious presence of a strong bar feature across the central region. There are no clear signs of a major merger event, although there might be some minor distortions in the spiral arm structure suggestive of interactions. The galaxy exhibits a range of stellar populations, inferred from the color variations, with bluer regions likely indicating younger, hotter stars and redder regions suggesting older stellar populations.