The galaxy presents as a single, relatively symmetrical, smooth and concentrated distribution of light. The light profile appears centrally concentrated with a bright core that diffuses outwards. The galaxy displays an elliptical morphology, appearing nearly circular, showing little or no evidence of spiral arms or a galactic disk. There is a subtle color gradient, showing a slightly redder hue towards the core. There is no significant presence of tidal features, dust lanes or irregular structures in the visible light, which suggests that the galaxy may be in a relatively quiescent state, without major ongoing mergers or starburst activities.
