The galaxy presents as an elliptical morphology, appearing largely smooth with a subtle disk feature possibly in the process of formation. The galaxy exhibits a central bulge that appears bright and concentrated, surrounded by a more diffuse halo of starlight. The color profile suggests a population of older stars, as the galaxy shows a reddish-yellow hue typical of galaxies where star formation has slowed or ceased. There is some minor disturbance to the symmetry of the light distribution, suggesting the possibility of a past interaction. The galaxy appears slightly elongated.
