This galaxy appears to be a relatively smooth, centrally concentrated system, consistent with an elliptical morphology. There is a distinct color gradient, with the core exhibiting a yellowish-white hue suggestive of an older stellar population. The outer regions of the galaxy appear redder, indicating a population of evolved stars and possibly a lower rate of ongoing star formation.

The galaxy shows a slight deviation from perfect circularity, leaning towards a slightly elongated shape. There is no readily apparent evidence of spiral arms or other distinct features. No major disturbances or mergers are apparent in the image, supporting the view that this galaxy has likely undergone relatively undisturbed evolution recently.
