The galaxy presents as an elliptical structure, exhibiting a high degree of central concentration. Its morphology appears largely smooth, lacking any prominent spiral arms or distinct disk features. The color profile shows a primarily yellow-orange hue concentrated towards the galactic center, indicative of an older stellar population. A subtle color gradient exists, with slightly bluer tones present in the outer regions relative to the core. There is no immediately observable evidence of active galactic nuclei activity. Overall, the galaxy appears to be in a relatively quiescent state, without any major signs of ongoing mergers or significant star formation. The overall round shape suggests minimal rotational support.
