The galaxy presents as a smooth, elliptical-like structure, though potentially disturbed. A brighter, more concentrated central region is evident, suggesting a prominent galactic nucleus. The overall color appears relatively uniform, with a subtle shift towards redder hues. This implies an older stellar population, with relatively low levels of ongoing star formation. The galaxy may be undergoing a merger, as evidenced by the irregular overall shape. There is a second area of brightness, lending credence to a merger event.
