This galaxy presents as a luminous, elliptical-like structure, appearing relatively smooth in texture. The core is intensely bright, exhibiting a reddish hue, possibly indicative of an older stellar population and diminished recent star formation. Fainter, diffuse greenish emissions extend outwards from the central region. The lack of distinct spiral arms or prominent dust lanes suggests that this galaxy is unlikely to be a spiral galaxy, but rather an early-type galaxy transitioning slowly from star forming to quiescent. There is evidence of some disturbed morphology, although the galaxy is not undergoing a major merger event, as there is no defined other structure. 
