The galaxy exhibits a complex morphology, with evidence suggesting an ongoing or recent interaction or merger event. The primary component appears somewhat amorphous, lacking a clear spiral or elliptical structure. There is a brighter, more concentrated region within the galaxy, possibly representing the core or bulge. Adjacent to this, there appears to be a distinct secondary component, suggestive of another galaxy in the process of merging. The color profile indicates the presence of both older stellar populations, visible as yellow and orange hues, and potentially some regions of ongoing star formation, suggested by bluer tints. The system displays moderate disturbances in its overall shape, further supporting the interaction scenario. Faint tidal features may be present, though difficult to discern definitively.
