This galaxy appears to be undergoing a merger event. It presents an overall elliptical morphology, with what appears to be a central bulge and a disrupted or disturbed disk. The light distribution suggests a redder, more centrally concentrated component, and a bluer, more diffuse component. 

There is a noticeable asymmetry and irregularity in the shape, possibly due to tidal interactions. The central region presents a more uniform color, while the outer regions suggest some degree of clumping or knotty structures, potentially regions of star formation triggered by the merger. The overall appearance indicates a system that is not fully relaxed, and the merger is in a relatively advanced stage, but not yet fully coalesced.
