The galaxy appears to be a relatively smooth, elliptical system. Its light profile suggests a high degree of central concentration, typical of elliptical galaxies. There is no evidence of spiral arms or a distinct disk structure. The galaxy displays a uniform color gradient, shifting from a bluer core region to redder outer regions. The shape is close to circular with no strong indication of tidal features or other signs of recent mergers. Based on the redder color of the outer regions, it may have an older stellar population. The high degree of smoothness suggests a relaxed morphology, possibly indicating a relatively quiescent evolutionary history. 
