The galaxy appears to be a spiral galaxy, though the spiral arms are somewhat disturbed or ill-defined. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population. Faint blue regions are observed within the disk, indicating the presence of younger, hotter stars and potential ongoing star formation. The overall shape is moderately elongated. There is potential evidence of minor disturbances present in the spiral arms, perhaps hinting at a possible interaction or recent minor merger event. The smoothness fraction is high indicating a largely smooth structure, there is a significant fraction of intermediate roundness. Overall, the galaxy is transitioning between a smooth elliptical shape and a fully-developed spiral structure.
