The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy, though some minor disk features may be present. Its light profile suggests a dominant spheroid component. The galaxy has an overall round appearance, although there appears to be a slight elongation, possibly due to rotation or tidal forces. There's a subtle color gradient, appearing slightly bluer towards the outer regions, which could be indicative of younger stellar populations in the outskirts. There are no obvious signs of major ongoing mergers or significant tidal disturbances. It has an apparent size that suggests this is a very large galaxy. Given the galaxy's significant mass and lack of active star formation, this is likely a well formed galaxy in its mature state.
