The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless structure at this resolution. It has a prolate shape with an intermediate ellipticity. The central region displays a yellowish-white hue, suggestive of an older stellar population. Moving outward, there's a subtle color gradient toward the edges, showing some bluer tones indicating some presence of younger stars toward the galactic outskirts. There is little to no evidence of spiral arms or distinct dust lanes within the galaxy's structure. The overall appearance indicates a galaxy that has undergone significant evolution, possibly having exhausted much of its gas reservoir for ongoing star formation.
