The galaxy presents as a relatively smooth, elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-orange hue, suggesting a population of older stars. The overall light distribution indicates a high degree of radial symmetry with minimal discernible substructure such as spiral arms or prominent dust lanes. Faint extensions of diffuse light are observed surrounding the central region, indicating an extended stellar halo. There is an object near the galaxy that could be a companion galaxy, or perhaps a background object. Based on the smoothness of the overall galaxy, it appears to be a quiescent system with low star formation.
