The galaxy presents a largely smooth morphology, exhibiting a centralized concentration of light. It is nearly circular, deviating slightly from a perfect spherical shape, tending more towards an elliptical form. There is a clear color gradient apparent, with the central region appearing redder in comparison to the outer edges, which exhibit a greenish hue. The galaxy displays no obvious signs of spiral arms or significant dust lanes, nor is there any readily apparent evidence of ongoing merging activity or major disturbance in its structure. The galaxy appears as a singular, well-defined object, with a notable lack of pronounced substructure within the available resolution.
