The galaxy presents as a spiral type, with a clear disk structure viewed at an oblique angle. Two spiral arms are distinctly visible, exhibiting a loosely wound morphology. The central bulge appears moderate in size, showing a yellowish hue which indicates an older stellar population. The arms display clumpy regions, suggestive of active star formation regions. There is no obvious presence of a strong central bar. No signs of major mergers, or other signs of significant gravitational interaction are readily apparent.
