The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, primarily featureless morphology, with no prominent spiral arms or bar structures discernible. The light distribution is fairly regular, with a gradual decline in intensity from the core outwards. The galaxy's color appears to be generally yellowish, suggesting an older stellar population with a dearth of ongoing, high-rate star formation. There is a hint of bluer light near the center. Overall the galaxy's structure does not suggest a strong history of past mergers, or currently undergoing a merger.
