The galaxy presents as a moderately luminous, elliptical structure with a slight disclike bulge. It exhibits a smooth, relatively featureless morphology, lacking distinct spiral arms or prominent dust lanes. The central region is characterized by a bright, concentrated core, suggesting a high stellar density. The color profile indicates a population of older stars, which are primarily concentrated in the core, transitioning to younger stars in the outer layers.

There are indications of possible minor disturbances in the outer regions of the galaxy, which could be tidal features. The roundness of the central bulge appears mostly spherical, while the entire galaxy seems to be in between spherical and elliptical shape.
