This galaxy presents as a spiral type, exhibiting a distinct disk structure with prominent spiral arms. The arms appear flocculent and well-defined, tracing a relatively grand design morphology around the central bulge. The winding of the spiral arms is of medium tightness. A notable feature is a bar-like structure that traverses the central region.

The bulge appears moderate in size, contributing significantly to the galaxy's overall luminosity, particularly in the central region. The disk shows evidence of ongoing star formation, evidenced by the presence of bluer regions within the spiral arms. Dust lanes are visible, particularly along the inner edges of the spiral arms, obscuring some of the light from behind. The overall color of the galaxy is indicative of a mix of stellar populations, with the bulge showing a yellowish hue, suggesting an older stellar population, while the arms are bluer, indicating younger, hotter stars.

There is some indication of gravitational interaction or disturbance, possibly from a minor merger, with asymmetries visible in the outer disk.