The galaxy presents as a relatively smooth, featureless object. Its shape appears intermediate between round and elliptical, with a slight elongation. A color gradient is observable, transitioning from a yellowish core to a slightly bluer outer region. This color variation suggests potential differences in stellar populations, with the core possibly dominated by older, redder stars, and the outer regions exhibiting younger, bluer stars. There is no evidence of a spiral structure or any major merger events. Slight irregularity within the extended halo is possibly indicative of a minor disturbance from a merger or tidal interaction. Based on its overall morphology, it appears to be a mature galaxy with signs of a past interaction.
