The object presents as a single, centrally concentrated galaxy. It appears largely smooth in texture, with a high degree of central luminosity that diminishes gradually towards its outer edges. The morphology is generally elliptical, showing a near-perfect rounded profile. No discernible spiral arms, bars, or obvious dust lanes are visible. There is no major or minor merging activity present or tidal disturbance evident in the image. The light profile suggests a relatively quiescent or evolved system, potentially with a population of older stars dominating the central region. A faint, diffuse halo may be present around the bright central core, but the image resolution limits a definitive assessment of its structure and composition.
