The galaxy presents an overall elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a bright, yellowish hue, suggesting an older stellar population. The galaxy's outskirts appear less defined, with a gradual fading of light intensity from the center outward. There is a slight elongation along one axis, indicating a deviation from perfect sphericity. Subtle disturbances or asymmetries in the outer regions suggest possible past interactions or merging events, although the main body of the galaxy appears relatively undisturbed. Faint hints of spiral structure or disk-like features cannot be entirely ruled out based on the image alone, but the dominant characteristic is that of a smooth, spheroidal system.
