The galaxy appears to be a relatively smooth, elliptical system. Its color suggests an older stellar population, with a dominant yellowish hue concentrated centrally. There is little evidence of spiral arms or distinct disk structure. The galaxy exhibits a high degree of central concentration, with brightness decreasing smoothly towards its outer edges. The morphology is predominantly spheroidal with a high degree of roundness. There is no obvious signs of any major mergers or disturbances. The galaxy's overall appearance indicates a quiescent, possibly early-type system.
