The galaxy presents as a somewhat elliptical structure, with a high degree of central concentration. The light distribution appears relatively smooth, lacking any pronounced spiral arm features or distinct dust lanes. There is a slight elongation, suggesting a possible transition between elliptical and lenticular morphology. The core exhibits a yellowish-white hue, potentially indicating an older stellar population, with a gradual fading to a bluer color towards the outer regions of the galaxy. This color gradient might suggest ongoing, though subdued, star formation activity within the galaxy, particularly in the outer disk. The overall form appears relatively undisturbed, lacking any obvious signs of recent major mergers or tidal interactions.
