The galaxy presents a largely smooth, elliptical morphology with minimal discernible features. The light profile is concentrated, with a bright, yellowish core that gradually fades into the outer regions. The overall shape appears close to circular, showing a high degree of roundness. There is no strong evidence of spiral arms, bars, or significant tidal disturbances indicating recent major mergers. The color suggests a stellar population dominated by older stars, potentially indicating low ongoing star formation.
