The galaxy presents as a well-defined elliptical structure, exhibiting a moderate degree of flattening. The light distribution appears centrally concentrated with a smooth, diffuse halo extending outwards from the core.  The color gradient suggests an aging stellar population, with a yellowish-white core indicative of older stars and a bluer outer region, potentially indicating ongoing, though subdued, star formation.  There is some indication of subtle disturbances, but nothing to suggest a recent major merger. The morphology of the galaxy is predominantly smooth and rounded.
