The galaxy presents a distinct spiral structure. The central bulge appears moderately sized and exhibits a yellowish hue, indicating a likely population of older, cooler stars.

The spiral arms are prominent and extend outwards from the central bulge. They appear relatively tightly wound, tracing a well-defined pattern. The bluer color in these arms suggests ongoing star formation and the presence of younger, hotter stars. The galaxy's disk appears largely unperturbed, with no immediately obvious signs of major merger activity, though some minor disturbances cannot be ruled out. Overall, the galaxy appears as a well-formed spiral galaxy, possibly with two dominant spiral arms.