The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely rounded in shape. Color gradients suggest a redder core region that gradually transitions to a bluer outer halo. No distinct spiral arm structures or significant dust lane features are discernible from this image. There appears to be little to no signs of any major merger events or tidal disturbances in its morphology. The galaxy demonstrates overall smoothness, suggesting it is likely a relatively settled system. The light distribution indicates a higher density of older stars in the center, with younger stars contributing to the bluer color of the outer regions. This galaxy is likely undergoing relatively little star formation.
