The galaxy presents as a spiral with a moderate central bulge. The spiral arms are prominent but somewhat flocculent, displaying a distinct blue hue, suggesting ongoing star formation. The arms exhibit a winding pattern that appears primarily tight to medium, with hints of multiple arm structures, possibly four or more. No obvious bar feature is discernible. There is no prominent evidence of a major ongoing merger, although some subtle irregularities or minor disturbances may be present within the disk. Overall, the galaxy appears well-defined.
