This galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a slightly elongated, disk-like morphology, but lacks obvious spiral arm structures. The central region shows a bright, somewhat diffuse yellowish-white glow, suggesting the presence of an older stellar population and possibly a supermassive black hole. The outer regions fade in intensity, showing a redder hue, possibly indicating the presence of older stars or dust obscuration. Minor asymmetries or subtle disturbances are barely perceptible in the galaxy's structure.
