The galaxy displays a complex morphology, appearing as a system with multiple components. A brighter, relatively compact central region exhibits a smooth, elliptical profile with a hint of greenish coloration suggesting the presence of ionized gas or recent star formation. Extending from this core is a fainter, more diffuse structure resembling a tidal tail. This tail is elongated and exhibits a bluish hue, potentially indicative of younger stars or a lower metallicity stellar population. This structure suggests the possibility of a past or ongoing interaction or merger event. Overall, the galaxy is relatively blue, suggestive of active star formation, though some regions exhibit a more yellow/red coloration, likely associated with older stellar populations. 
