The galaxy appears to be elliptical in shape, exhibiting a high degree of central concentration. The light distribution is smooth and lacks prominent features such as spiral arms or a distinct disk. There is a slight elongation. The color gradient suggests a population of older stars, with a yellowish hue dominating the galaxy's composition. There is no apparent active galactic nucleus or significant dust lane. The overall morphology is indicative of a quiescent, evolved system. There are no obvious signs of recent or ongoing merger activity, though subtle irregularities in the outer isophotes could suggest a minor interaction in the past.
