The galaxy presents as an elliptical morphology, appearing largely smooth and relatively featureless. The central bulge is bright and concentrated, exhibiting a yellowish hue, suggesting a population of older stars. The galaxy's light gradually diminishes toward its outer edges, forming a diffuse halo. There is a slight hint of a disk-like structure, however, it is difficult to see clearly. Overall, the galaxy appears largely undisturbed, showing no major signs of ongoing mergers or tidal interactions. 
