The galaxy exhibits a smooth, centrally concentrated light distribution. It appears elliptical in shape, though some slight deviations from perfect elliptical symmetry cannot be ruled out due to the image quality. The galaxy's color gradient is subtle, showing a slightly more yellow hue in the central regions, likely indicating an older stellar population and a lack of significant ongoing star formation in the nucleus. There is no discernible evidence of spiral arms or a disk-like structure. Overall, the galaxy's morphology suggests it is a relatively evolved system, potentially a massive elliptical galaxy which has undergone some past mergers. There is no strong indication of tidal features or ongoing mergers.
