The galaxy exhibits a disk-like morphology, although some degree of disturbance is evident. Spiral arm structures are discernible, appearing somewhat patchy and not well-defined. A central bulge is present, but it does not appear to dominate the overall structure. The galaxy displays a color gradient, with the central regions appearing more yellow/red, suggesting an older stellar population, while the outer regions exhibit a bluer hue, potentially indicating ongoing star formation. Overall the galaxy appears to be undergoing some type of galactic merging process.
