The galaxy presents as a relatively smooth, centrally concentrated object. The color gradient suggests a bulge-dominated morphology, transitioning from a bright, yellowish-white core to a more diffuse, bluish-tinged outer region. No distinct spiral arm structures or other significant features are immediately apparent. The overall roundness indicates a possible elliptical or lenticular classification, with minimal distortion suggesting a quiescent state in terms of major mergers or tidal interactions. There is a slight elongation, indicating that it is not perfectly circular. The galaxy is exhibiting low star formation.
