The galaxy presents as a moderately inclined spiral with a discernible disk structure. Spiral arms are visible, exhibiting a somewhat flocculent morphology, with medium winding. The central bulge appears neither overly prominent nor diminutive, suggesting an intermediate bulge-to-disk ratio. The disk shows evidence of blue-shifted regions, particularly within the spiral arms, indicative of ongoing star formation activity. A slight asymmetry is noted in the outer regions of the disk. The galaxy does not appear to be strongly barred. Overall, the galaxy exhibits characteristics consistent with a normal spiral galaxy undergoing active star formation.
