The galaxy presents a complex morphology, displaying characteristics of both a smooth spheroid and disturbed features. The primary body of the galaxy exhibits a relatively smooth, elliptical profile, suggesting an evolved stellar population. However, there are also distinct indications of tidal disturbances or interactions. A faint plume or tail-like structure extends from one side of the galaxy. Within the galaxy itself, there appear to be areas of enhanced star formation, indicated by the patchy, irregular distribution of bluer regions. A significant portion of the galaxy appears redder, indicating older stars. The overall impression is of a massive galaxy undergoing or having recently undergone some form of interaction or merger event that is driving localized star formation and disrupting its otherwise smooth structure.
