The galaxy presents as a somewhat elliptical, relatively smooth distribution of light, with a concentrated central bulge. The core exhibits a yellowish hue, possibly indicating an older stellar population. Fainter bluish light extends outwards from the central region, suggesting the presence of younger, hotter stars in the galaxy's outer regions, where some star formation may be occurring at a low rate. There is a subtle hint of a disk-like structure, but the overall form is more akin to an elliptical or lenticular galaxy. Some minor disturbances may be present, suggesting a possible past interaction or merger event. The galaxy is not perfectly spherical, exhibiting a slight elongation, with an estimated effective radius of a few kiloparsecs.
