The galaxy presents as a relatively smooth object, with a somewhat elliptical morphology. There is a slight elongation, but the structure is primarily rounded. The color gradient suggests a redder core, fading to bluer outer regions. The lack of distinct spiral arms or a prominent bulge points towards a later-type classification, possibly an elliptical or lenticular galaxy with a relatively low star formation rate. There might be some minor disturbances or tidal features hinting at a past interaction, but no major merger events are apparent. The overall structure indicates a galaxy that is primarily dominated by older stellar populations.
