This galaxy exhibits a generally smooth morphology. It appears to be elliptical in shape, with a high degree of central concentration. There is a bright, yellowish core which fades gradually into the outer regions. The colour gradient suggests a population of older stars dominating the central bulge. Fainter extensions around the galaxy are visible but lack any discernible structure, suggesting a smooth stellar halo. There is no indication of prominent spiral arms or active star formation regions visible in the image. The overall appearance indicates a galaxy that has undergone substantial aging of the stellar population. Evidence suggests it has likely ceased major star forming activity. There are no signs of a major ongoing merger.
