The galaxy presents as a relatively smooth, centrally concentrated light distribution. There is no apparent spiral structure or bar. The galaxy exhibits an elliptical morphology, appearing mostly round. Color gradients within the galaxy are subtle, with a slightly bluer core possibly indicating recent or ongoing star formation. There are no signs of tidal tails or other strong gravitational disturbances. The overall appearance suggests a mature galaxy with a substantial stellar mass and a relatively low star formation rate. It is likely a quiescent system.
