The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a noticeable color gradient, transitioning from a bright yellowish-white core to a bluer, fainter outer region. The galaxy's shape is slightly elongated. There is little evidence of significant dust lanes or spiral arm structures. It appears relatively undisturbed, without signs of major recent merger activity. The color profile suggests a population of older stars dominating the central region, with potentially younger, bluer stars contributing to the outer halo.
