The galaxy presents an overall elliptical morphology with a suggestion of tidal disturbances and ongoing interactions. The central region is dominated by a bright, concentrated core exhibiting a yellowish-white hue, potentially indicative of an older stellar population. Extending outward from the core, the galaxy displays a more diffuse halo, exhibiting a gradient in color, shifting towards redder tones. At least one distinct, bright clump of material is visible, appearing separated from the main body of the galaxy. This clump shows a bluer color, suggestive of more active star formation. The overall structure implies a system undergoing, or having recently undergone, a merger event, resulting in the observed morphological distortions.
