This galaxy presents a notable disk structure, viewed at an oblique angle that suggests it is nearly edge-on. The disk component appears to be the dominant feature, displaying characteristics indicative of spiral arms. Although the spiral structure is somewhat disrupted and asymmetric, the winding appears to be generally medium to loose.

A moderate bulge is discernible, though it is not overly prominent. The central region of the galaxy exhibits a yellow to orange hue, suggestive of an older stellar population, while the outer regions of the disk show bluer regions, potentially indicative of ongoing star formation. 

There is evidence of disturbances within the galactic structure. Areas of more pronounced asymmetry suggest possible tidal interactions or past minor mergers. The disk exhibits clumpy regions. Furthermore, the presence of a bar structure may be contributing to the irregularity observed in the spiral arms. The overall morphology suggests a galaxy undergoing active star formation within its spiral arms and disk.