The observed galaxy presents an overall elliptical morphology. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or other distinct features typically associated with disk galaxies. The galaxy exhibits a color gradient, appearing bluer in its outer regions and redder towards its core, suggesting a stellar population gradient and potentially ongoing star formation in the periphery. There is some visual evidence of asymmetry, with a slight elongation or possible tidal feature extending from one side. The galaxy displays a diffuse halo, possibly indicative of past merger activity or stellar stripping.
