This galaxy exhibits a largely elliptical morphology, appearing smooth and relatively featureless in its overall structure. The light distribution suggests a high degree of central concentration, with a bright core fading gradually outwards. There is a hint of a disk component, but it is faint and subtle. The galaxy appears mostly round. The color index suggests the presence of an older stellar population, with a redder overall hue and a relatively low star formation rate. There are no indications of major tidal disturbances or ongoing mergers, though the possibility of minor interactions cannot be entirely ruled out. The light is consistent with an object with a substantial mass.
