The galaxy presents an elliptical morphology, exhibiting a smooth light distribution. The central region displays a concentration of light with a yellow hue, potentially indicative of an older stellar population. Surrounding the core, there is a gradual decrease in surface brightness, with a bluish halo extending outwards. The galaxy appears to be in a relatively undisturbed state, showing no obvious signs of major merger activity, although there may be a minor irregularity in the outer regions that suggests a possible past interaction. Overall, the galaxy appears to be a relatively smooth system without prominent spiral arm structures.
