The galaxy presents as a luminous, centrally concentrated object. Its overall morphology appears largely smooth and elliptical. The core exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outwards from the center, the color profile shifts subtly towards a slightly greener tint, potentially indicating a small amount of younger stars or ongoing star formation, though it is very subdued. There are no distinct spiral arms or a clear disk-like structure visible; instead, the light gradually fades away from the center. The galaxy appears relatively undisturbed, lacking any signs of major tidal interactions or recent mergers, though there may be some minor disturbances given the slight irregularity of the light distribution on the outskirts. The galaxy presents with a notably round appearance. Overall, the morphology is consistent with a galaxy towards the red sequence, likely a massive elliptical galaxy with a low star formation rate.
