The galaxy exhibits a disk-like morphology, although it is not clearly defined. The central region appears brighter and more concentrated, suggesting the presence of a bulge. There is evidence of spiral arm structure, but it is somewhat faint and disrupted. The color distribution indicates the presence of both older stellar populations, visible as reddish hues, and younger, bluer stars, scattered throughout the disk and potentially within the spiral arms. Some irregularities in the shape and light distribution are noticeable, possibly indicative of minor gravitational interactions or internal disturbances. Overall, the galaxy appears to be transitioning between a smoother elliptical and a more defined spiral morphology, and may be in a state of minor disruption. 
