The galaxy presents as a centrally concentrated spheroid. It displays a smooth, mostly uniform luminosity profile, appearing elliptical in shape. The core region exhibits a yellowish hue, suggesting an older stellar population. The outer regions fade into a faint blue/green color gradient with distance from the core, indicating the presence of some younger stars and potential ongoing star formation. There's no evidence of spiral arms, bars, or any major tidal disturbances that would indicate recent merger activity. Overall, this galaxy appears to be an evolved system.
