The observed galaxy presents a relatively compact structure with a bright, concentrated central region. The color profile suggests a gradual transition in stellar populations moving outwards from the core. The inner core exhibits a bluish-white hue, potentially indicative of hotter, younger stars and ongoing star formation. Surrounding this core is a greenish halo that could signal a mix of stellar populations. The outer regions display a subdued blue tint. Overall, the galaxy appears to be fairly symmetric, with no immediately apparent signs of significant tidal disturbances or major merger events. Some minor morphological asymmetries in the halo suggest a slight disturbance. The object is generally categorized as a smooth galaxy, and that it does not have a clearly defined disk-like structure.
