The galaxy presents a distinct disk morphology. Evident spiral arm structures are present, exhibiting a loosely wound pattern. Two prominent spiral arms are observed. A central bar feature is discernable, bisecting the galaxy's core. The bulge appears to be of moderate size, contributing significantly to the overall galactic structure. The galaxy exhibits a generally undisturbed appearance, although possible indications of minor disturbances or interactions cannot be ruled out completely. The galactic disk presents variations in color, implying differing stellar populations and/or dust obscuration. Overall, the galaxy can be classified as a barred spiral galaxy.