The galaxy presents as a singular, luminous object with an elliptical morphology. The light profile appears smooth and centrally concentrated, with no readily discernible spiral arm structures or prominent dust lanes. The galaxy's color suggests a more evolved stellar population, with a bias towards redder wavelengths, indicative of older, cooler stars. There may be very minor signs of a disturbance, but the galaxy appears mostly relaxed. The overall structure indicates a well-established system, likely a spheroidal galaxy with a substantial stellar mass.
