The galaxy presents as a relatively smooth, elliptical structure. Its morphology suggests a system that is not actively undergoing a major merger, though a minor disturbance cannot be ruled out. The galaxy exhibits a high degree of central concentration, with the majority of its light emanating from a bright, somewhat diffuse core. The overall color appears to be redder, indicative of an older stellar population with less ongoing star formation. The shape is more akin to an in-between roundness and cigar shape. Based on these characteristics, the galaxy appears to be a fairly massive system.
