The galaxy appears to be a disk galaxy, observed at a relatively high inclination angle. There is a central bulge region that is relatively prominent and appears smooth and concentrated. The disk component exhibits a somewhat irregular morphology, suggesting the presence of spiral arm structures, although they are not sharply defined. The color gradient suggests some active star formation, particularly in the disk, where bluer hues are visible. The overall light distribution suggests a mature galaxy with a significant population of older stars in the bulge and ongoing star formation within the disk. Some disturbances appear to be visible, but they are minor. The disk seems relatively uniform in color and brightness across its structure.
