The galaxy presents as a centrally concentrated object with a relatively smooth, elliptical morphology. A slight color gradient is visible, with a hint of bluer tones in the innermost region, gradually shifting towards redder hues in the outer parts. It displays a high degree of central concentration and a moderate axial ratio, appearing somewhat flattened. The overall structure suggests a mature system, though subtle color variations indicate ongoing, low-level star formation activity within the core. No pronounced spiral arms or distinct features are discernible. The galaxy's light profile appears well-fit by a de Vaucouleurs profile.
