The galaxy presents as a slightly elongated, centrally concentrated object. Its morphology appears to be smooth and relatively featureless; there is no apparent spiral structure, bar, or dust lane visible in this image. The galaxy exhibits a color gradient, with a yellowish-white core gradually transitioning to a bluer hue at the outer edges. This suggests a moderate amount of ongoing or recent star formation, particularly in the outer regions. The overall appearance is consistent with an elliptical or lenticular galaxy, exhibiting a degree of rotational symmetry and lacks any signs of major tidal disturbances or ongoing mergers. The galaxy appears well-defined against the background, and its diffuse halo extends noticeably outwards, hinting at a substantial mass.
