This galaxy presents a clear disk morphology. It has well-defined spiral arms, with a distinct winding pattern. Two spiral arms are very obvious. The arms exhibit a clumpy texture, suggesting regions of active star formation. The central bulge appears moderate in size with a yellowish colour and could have older stellar populations. There is no obvious sign of any bar or any major merger activity disrupting the disk. The inclination is close to face-on. The colour profile indicates a higher concentration of younger, bluer stars within the arms, contrasting with the older, redder population likely concentrated in the bulge.
