The galaxy presents as a relatively smooth, elliptical structure, displaying a concentrated central bulge with a diffuse halo. There is a slight elongation in shape. The color profile suggests an older stellar population, with a dominant yellowish hue in the central regions, indicating a population of evolved stars. A subtle gradient towards bluer colors is observed in the outer regions of the halo, potentially signaling pockets of younger stars. The absence of well-defined spiral arms or prominent dust lanes indicates a classification as an early-type galaxy. There are no apparent signs of major interactions or ongoing mergers.
