The observed galaxy presents as a relatively smooth, centralized object. Its morphology suggests a predominantly spheroidal structure, displaying minimal discernible disk features or spiral arms. The overall light distribution appears concentrated towards the center, indicating a prominent galactic bulge. There is little indication of ongoing major mergers or significant tidal disturbances in its immediate vicinity. The color profile suggests a population dominated by older stars, with a weak blue component, indicative of a low star formation rate.
