The galaxy presents as an elliptical structure with a smooth light distribution, with an indication of a possible disk-like feature. The central region exhibits a bright core, surrounded by a yellowish ring-like structure, indicating older stellar populations. Beyond the core, the galaxy displays a transition towards a fainter, bluer outer region, suggesting the presence of younger stars. A small area of redder light appears outside of the ring, with a handful of others scattered in the galaxy's outer reaches, potentially indicative of areas of dust obscuration or older stellar populations. The galaxy appears moderately elongated. There's no obvious sign of a recent major merger, but the morphology suggests a possible past interaction that has disturbed the round shape.
