The galaxy appears as a luminous, elliptical-shaped structure, exhibiting a smooth and relatively featureless morphology. The core presents a bright, concentrated emission, gradually fading into the outer regions. The color distribution suggests an older stellar population, likely dominated by redder, evolved stars. There is little evidence of ongoing, active star formation within the galaxy. The galaxy's shape indicates a system in equilibrium, without significant signs of recent mergers or tidal disturbances.
