The galaxy presents as a smooth, elliptical morphology with a highly concentrated central bulge.  The outer regions fade gradually into the background, suggesting a lack of distinct spiral arms or prominent dust lanes.  The color profile indicates a dominant population of older stars, exhibiting a yellowish-red hue in the outer regions shifting to bluer tones in the inner regions. There are subtle irregularities in the outer isophotes, which might suggest past minor interactions or accretion events but generally these are quite smooth and even. Overall, the galaxy appears relatively undisturbed and evolved.
