This galaxy exhibits a complex morphology suggesting an ongoing or recent interaction with another galactic body. The primary structure appears largely spheroidal, exhibiting a diffuse, relatively smooth light distribution. A noticeable color gradient is present, with the central region displaying a bluish hue, suggestive of a population of younger, hotter stars. Adjacent to the primary structure, a distinct yellowish or reddish component can be observed, potentially indicating an older stellar population. The overall shape deviates from a perfect ellipse, hinting at tidal disturbances. A significant portion of the galaxy's light is concentrated within a relatively small radius, but the outer regions are noticeably disturbed. There appears to be light distribution that may indicate a galactic merger event.
