The galaxy presents as a diffuse object, appearing neither definitively elliptical nor clearly spiral. It exhibits a moderate degree of central concentration, with a relatively smooth, gradual transition from the core to its outer regions. The light distribution suggests a primarily spheroidal component. The galaxy displays a yellowish hue, potentially indicating an older stellar population with fewer young, massive stars. There is a suggestion of minor disturbance within the galactic structure, possibly indicating a past interaction or merger event. Overall, the galaxy's morphology points towards an intermediate stage of evolution, lacking prominent spiral arms and exhibiting a relatively high degree of spheroidal dominance. 
