The galaxy presents as an elliptical morphology, characterized by a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, which likely indicates an older stellar population with diminished recent star formation. Moving outwards from the core, a gradual decrease in surface brightness is observable. The outer regions display a more greenish tint, which could result from a tenuous scattering of light or a sparse population of younger stars. The galaxy appears slightly elongated with a major axis that is roughly aligned in a northwest-southeast direction. Subtle irregularities or disturbances may be present in the outer regions, potentially indicating minor tidal interactions or past merger events. Overall, the galaxy shows a relatively regular structure, consistent with an evolved system in a post-starburst phase.
