The galaxy presents an overall elliptical morphology, although with hints of a possible disk structure. Its light profile suggests a relatively smooth distribution, potentially indicating an older stellar population dominating its composition. The central region is brighter and more concentrated, possibly indicative of a galactic bulge. The color profile shows a bluish central region surrounded by a yellower disk. The galaxy appears to be undergoing some form of interaction, displaying minor tidal disturbances. Overall, it seems to be in a transition between the stages of the assembly history. 
