The galaxy presents as a relatively compact object, displaying a somewhat irregular morphology. A central, bright core is visible, surrounded by a diffuse halo. There is evidence of some disk-like structure but no clear, defined spiral arms, or well defined bar. The central region exhibits a cyan color. Redder hues appear in the periphery, indicating either older stellar populations or dust obscuration. Overall, the galaxy appears to be in a disturbed state, possibly indicating an ongoing or recent interaction or merger event.
