The galaxy appears to be an elliptical galaxy, likely located at a considerable distance based on its small apparent size. It exhibits a smooth, centralized light distribution with a minimal presence of spiral arm structures or dust lanes. The core of the galaxy is bright and concentrated, transitioning smoothly to a fainter halo. There is a slight elongation in the shape, suggesting a deviation from perfect circularity. The color gradient suggests a population of older stars. There may be evidence of minor disturbance, but it is negligible.
