The galaxy presents as a spiral structure with a central bulge. The spiral arms exhibit a relatively tight winding pattern, with discernible, though somewhat diffuse, blue star-forming regions distributed along the arms. The arms appear somewhat flocculent, lacking a sharply defined structure. There is some evidence of an inner spiral arm. The central bulge has a small, almost indistinct nature, appearing smooth and less prominent relative to the disk. The galaxy displays no obvious signs of a bar feature. Overall, the galaxy exhibits a generally symmetrical morphology.
