The galaxy presents a distinct spiral structure, with two prominent arms clearly visible. These arms exhibit a moderately wound morphology, suggesting an intermediate stage of spiral arm development. The color distribution within the galaxy indicates a mix of stellar populations. The central bulge shows a yellowish hue, potentially indicative of an older stellar population and a lower rate of star formation. The spiral arms, on the other hand, appear bluer, possibly indicating regions of ongoing star formation and younger, hotter stars. There is a hint of a bar-like structure across the bulge region, but it is not very prominent. Overall, the galaxy is relatively large and shows no obvious signs of major mergers.
