The galaxy exhibits a predominantly smooth morphology. The light distribution is relatively concentrated, suggesting a spheroidal or elliptical structure. The galaxy appears nearly circular. There are indications of disturbances in the morphology, possibly resulting from interactions or mergers. There are multiple galactic nuclei. A tidal tail is visible, indicating an ongoing or recent merger event. Color gradients are present across the galaxy, with a slight blue hue in the central regions and a redder color toward the outer edges. 
