The galaxy presents an elliptical morphology, appearing largely smooth and centralized. It displays a concentrated core region, brightest in the observed wavelengths. The overall color suggests a moderate age stellar population, leaning towards redder hues emanating from older stars. There's little evidence of distinct spiral arms or dust lanes. A slight elongation is visible, indicating a deviation from a perfect spherical shape. Minimal signs of on-going major interactions or disturbances are apparent within the galaxy's structure.
