The galaxy exhibits a flattened, disk-like morphology, although the structure is not sharply defined. The central region appears slightly brighter and more concentrated, suggesting the presence of a bulge. The color is predominantly a yellowish-white, hinting at a stellar population that is not dominated by young, blue stars. There are no prominent spiral arms or strong dust lanes readily visible in the image. Hints of some minor disturbances can be seen but the galaxy does not appear to be undergoing a major merger event. 
