The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing moderately rounded in shape, with no discernible spiral arm structures or prominent dust lanes visible in this image. The core region is a bright yellowish-white hue, which possibly suggests an older stellar population, consistent with a low specific star formation rate. The outer regions display a gradual decrease in surface brightness, exhibiting a diffuse, reddish halo, potentially indicative of a more metal-rich stellar population. There is no evidence of major morphological disturbances that might suggest recent or ongoing merger activity, though minor asymmetrical features may indicate subtle interactions. Overall, the galaxy appears to be a fairly quiescent, evolved system.
