The galaxy appears as a luminous, centrally concentrated object. Its morphology is generally smooth and elliptical, lacking discernible spiral arms or a distinct disk structure. The light distribution suggests a spheroidal shape, exhibiting a high degree of roundness. The core region demonstrates a significantly higher luminosity compared to its outer regions, potentially indicating a dense stellar population and a possible supermassive black hole at its center. The colors suggest a predominantly older stellar population, implying low levels of recent or ongoing star formation. There are no visually apparent signs of tidal disturbances, ongoing mergers, or major interactions with other galaxies.
