The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. The light profile appears relatively featureless, lacking prominent spiral arms or distinct dust lanes. The galaxy exhibits a moderate redshift, indicating a significant distance. Its color index suggests a population of older stars, although a slight bluer component is detectable, implying ongoing star formation. The galaxy is observed to be of substantial size and mass. There is no evidence of a major ongoing merger or significant tidal disturbance. The galaxy exhibits a slight degree of ellipticity, with a near-circular shape.
