The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears to be primarily spheroidal, with a high degree of central luminosity. There is a slight elongation visible, suggesting an elliptical rather than perfectly spherical form. The light profile appears to diminish gradually from the core outwards. The core region exhibits a yellowish-white color indicative of an older stellar population. Fainter, reddish hues appear in the outer regions, likely from more aged stars and potentially some dust. There are no prominent spiral arms or distinct features indicative of active star formation, suggesting the galaxy is relatively quiescent. There's no evidence of any significant mergers or tidal disturbances within the image.
