The galaxy presents as a somewhat elongated, lenticular-like system. A bright, concentrated central bulge dominates the overall structure, exhibiting a smooth, featureless appearance. Fainter light extends outwards from the core, forming a diffuse halo that appears more extended along one axis, suggesting an elliptical or possibly edge-on disk morphology. There is subtle color variation, with the central region appearing more yellow and the outer regions tending toward bluer hues. No distinct spiral arm structures or dust lanes are readily visible. There is no apparent evidence of strong tidal interactions or major merging events in this image, although some subtle asymmetries in the outer halo cannot be ruled out.
