This galaxy presents as an elliptical morphology, elongated in shape, with a noticeable color gradient from the center outwards. The central region appears a yellowish-orange hue, suggesting a population of older stars, while the outer regions exhibit a bluer tint, potentially indicating the presence of younger stars or regions of ongoing, though modest, star formation. There is no evidence of spiral arms or a well-defined disk structure. The galaxy exhibits a smooth appearance, with no major disturbances or signs of recent merging events visible. The overall structure indicates an evolved system with a significant fraction of its stellar population comprised of older stars, though some residual star formation may be present in the outer regions.
