The galaxy presents a flattened, elliptical morphology. The central region exhibits a concentrated, bright, yellowish hue, suggestive of an older stellar population. Moving outwards, the galaxy displays a more diffuse and bluish color, hinting at regions of ongoing star formation. There appear to be some disturbances in the structure, potentially indicative of minor gravitational interactions or an ongoing merger event. The spiral structure is not fully resolved, but there are hints of asymmetric features.
