The galaxy appears to be a relatively smooth, centrally concentrated elliptical galaxy at a redshift of approximately 0.24, indicating a considerable distance. It exhibits a nearly round morphology, with little to no evidence of a disk structure or spiral arms. The color profile suggests a dominant population of older stars, contributing to its yellowish-white hue in the central region. There is a subtle color gradient, with the core appearing slightly more yellow than the outer regions, potentially indicating variations in stellar population age or metallicity. There are no obvious signs of recent major mergers or significant tidal disturbances. The galaxy appears relatively undisturbed and well-defined.
