The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing more rounded than elongated. The light distribution appears fairly even, with a bright core that gradually fades into the surrounding halo. There is a hint of a slight disturbance or a faint arm-like feature extending from the main body, but the image resolution limits detailed assessment. The color gradient suggests a population of older stars, possibly with ongoing but limited star formation activity. The galaxy does not appear to be undergoing a major merger, although minor gravitational interactions cannot be entirely ruled out. Based on its apparent size and redshift, this is likely a massive galaxy.
