The galaxy appears to be a spiral, exhibiting a prominent disk structure. The spiral arms are well-defined and suggest a grand design morphology. There is evidence of a moderate bulge component at the center of the galaxy. The winding of the spiral arms ranges from tight to medium, indicating differential rotation within the disk. The galaxy has an overall blue color, which implies ongoing star formation. There are hints of dust lanes within the spiral arms, visible as dark patches against the starlight. The galaxy is not perfectly face-on, presenting a slightly inclined view relative to our line of sight. No major signs of tidal disturbances are visible. The bar is either weak or nonexistent.
