This galaxy appears to be a relatively smooth, disk-like structure. Its overall shape is somewhat elongated, showing a departure from perfect circularity but not exhibiting a highly distorted or cigar-like morphology. A central, brighter region is visible, suggesting a possible galactic bulge or nucleus. There's a subtle color gradient from the central region outward, potentially indicating varying stellar populations or dust distribution within the galaxy. The galaxy shows subtle features that may be spiral arms that are currently being disrupted by minor disturbances. This galaxy is also currently exhibiting a low star formation rate. There is no evidence of major merging events or interactions that would imply a major disturbance to the structure.
