The galaxy presents a generally smooth, elliptical morphology, exhibiting a high degree of central concentration. It appears largely featureless, lacking prominent spiral arms or a distinct disk. The color profile indicates a population of older stars, with a moderate presence of younger stars that contribute to star formation. The galaxy's shape is close to perfectly round. There is no evidence of any recent major or minor merger event, such as tidal tails or bridges, and no distinct visual disturbances.