The galaxy presents a distinct spiral morphology, characterized by two prominent, loosely wound spiral arms. The disk component appears to be the dominant feature. A central bulge is discernible, although it does not appear to be overly pronounced. The overall color suggests a mix of stellar populations, with bluer regions likely indicating ongoing star formation within the spiral arms. There may be signs of a minor interaction with a nearby object, showing small disturbances. The galaxy is not seen edge-on. There may be a weak bar, but it is difficult to tell for sure.
