The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated light profile, with the intensity decreasing gradually outwards from a bright, yellowish core. The overall shape is nearly circular, displaying little to no discernible disk-like structure or spiral arms. There is no clear indication of ongoing major merging activity or significant tidal disturbances. The color suggests a population of older stars and a lack of significant recent star formation, contributing to the galaxy's smooth appearance. There is a subtle color gradient observed, where the core appears slightly more yellow-orange compared to the outer regions which possess more greenish hues. Any internal structures appear blended at this resolution.
