This galaxy presents a distinct spiral morphology. The central bulge appears moderate in size and exhibits a yellowish-white hue, suggesting an older stellar population. A pronounced bar structure bisects the bulge, extending outwards into the spiral arms. These arms are well-defined and tightly wound, displaying a clumpy distribution of star-forming regions indicated by the numerous blueish knots visible along their lengths. The dust lanes appear dark. Overall, there are two distinct and prominent arms, while a couple more are barely there. There is no obvious major merger occurring; however, there are signs of minor disturbances within the disk, visible as slight asymmetries in the arm structure, likely indicating past or ongoing interactions. The galaxy's overall color gradient transitions from the yellow central bulge to bluer arms, indicative of younger star formation in the outer regions.
