This galaxy appears to be a spiral galaxy viewed at a significant inclination, though not quite edge-on. There is evidence of a disk structure with a brighter central bulge. The disk exhibits a mottled texture, suggesting the presence of star-forming regions. The bluer color in the outer regions of the disk indicates younger stellar populations and ongoing star formation. The bulge appears smoother and more yellow/red, indicative of an older stellar population. There are indications of minor disturbances. Based on its morphology, it is likely undergoing some sort of interaction with another galaxy. Overall, the galaxy displays characteristics of both a spiral and potentially an irregular galaxy due to the apparent disturbances.
