This galaxy presents as a relatively smooth, elliptical system. Its color profile is predominantly yellow and orange, suggesting an older stellar population with fewer young, blue stars. There is a slight elongation, but it appears largely spheroidal. No distinct spiral arm structures or dust lanes are discernible from this image. There seems to be a slight color gradient toward the center, with the core appearing more intensely yellow than the outer regions. The outer edges fade gradually into the background, indicating no sharp cutoff in stellar density. The apparent lack of significant substructure suggests a relaxed morphology, consistent with a galaxy that has undergone substantial internal homogenization.
