The galaxy presents as a spiral type with an observable disk structure. While somewhat disrupted, the disk exhibits hints of spiral arm morphology. There is a clear central bulge that appears relatively smooth and contains a yellowish hue, suggesting an older stellar population. The spiral arms appear clumpy, with regions of both bluish and reddish colors, indicating a mix of active star formation and older stars. Overall, the galaxy exhibits signs of possible minor disturbances in its morphology, and the spiral structure is somewhat irregular.
