The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall morphology suggests it is likely an elliptical galaxy, with a high degree of circular symmetry. The color profile is predominantly yellow/orange, indicating an older stellar population with a lower rate of current star formation. There are subtle hints of asymmetrical light distribution which may suggest a minor gravitational disturbance or interaction. Faint extended halo components surround the central core. The galaxy has an estimated size of approximately 9.5 kpc.
