The galaxy presents as a centrally concentrated, luminous object. Its morphology appears largely smooth with a possible subtle disc-like structure that is difficult to resolve. There is a slight deviation from a perfectly circular form. The color profile suggests a galaxy composed of older stellar populations. There is no strong evidence of recent star formation activity in the form of bright, blue regions. There are no obvious signs of interaction with other galaxies. However, a slight asymmetry may suggest a past interaction or minor disturbance.
