The galaxy appears to be a relatively smooth, elliptical-like structure. Its core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The light from the core gradually diffuses outwards, transitioning to a less intense, more diffuse halo surrounding the central region. There's a subtle color gradient, shifting from a warmer hue in the core to cooler tones in the outer regions. No distinct spiral arm features or dust lanes are discernible within the galaxy's structure from this perspective. There is no significant sign of tidal disruption or ongoing major merger events. The overall morphology suggests a system that is relatively relaxed and evolved.
