The galaxy presents a disk-like morphology, viewed at a significant inclination. A central bulge is discernible, appearing relatively smooth and concentrated. The disk exhibits a clumpy structure, hinting at the presence of star-forming regions. There is possible interaction with a smaller body in the lower right quadrant of the image, causing some distortion of the spiral arm structures. Dust lanes are visible within the disk, particularly along the inner regions, obscuring some of the starlight. The color gradient suggests a mix of stellar populations, with bluer regions possibly indicating younger, hotter stars and redder regions indicating older populations. Overall, the galaxy appears to be undergoing some form of disturbance or interaction, as evidenced by the clumpy disk and potential merger activity. The galaxy exhibits modest star formation activity. The estimated mass indicates it is a relatively small galaxy.
