This galaxy exhibits a complex morphology, potentially indicative of an ongoing or recent merger event. The overall structure appears disturbed, with a main, relatively smooth component displaying an elliptical shape. A secondary, less-defined structure is situated close to the primary, possibly representing a tidal tail or a smaller galaxy in the process of merging. There is a noticeable color gradient, with a more prominent orange hue indicative of an older stellar population. This contrasts with possible regions of active star formation that may be present, adding to the indication of interaction with another galaxy. The high degree of interaction suggests the likelihood of ongoing or recently ceased enhanced star formation activity within the system.
