The galaxy appears to be a relatively smooth, disk-shaped system, possibly an early-type spiral or lenticular galaxy seen at an oblique angle. The central bulge region exhibits a yellowish hue, suggesting an older stellar population. A hint of a flattened disk extends outward from the bulge. The disk shows a slight colour gradient, with bluer tones dominating the upper region, indicating the presence of younger stars or regions of active star formation. There is no clear spiral structure visible, the general appearance is disturbed and shows signs of potential merging.
