The galaxy presents a largely elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density. The light distribution appears relatively smooth with a subtle decrease in intensity as it extends outwards from the center, with faint redder hues on the outer edges. There is little apparent structure within the image, with no obvious spiral arms or prominent dust lanes visible, this further supports its classification as an elliptical galaxy. The galaxy does not display any obvious signs of major interaction or merging events, appearing as a single, relatively undisturbed object. The absence of strong blue light suggests a low rate of recent star formation.
