The galaxy appears to be a complex system, likely undergoing or having undergone a merger event. A significant portion of the galaxy exhibits a smooth morphology, appearing as a relatively featureless, roundish central component. However, there is also evidence of disturbance in the overall structure. We note at least two distinct bright areas that could be the cores of interacting galaxies. One such region shows a blue color, possibly indicating the presence of younger, hotter stars, suggesting ongoing star formation activity. A secondary yellowish region could be an older stellar population or a core. It is also possible that the blue region is in the process of merging with the primary object. A tidal tail or plume feature may be present and there are significant asymmetric light distributions around the galaxy. Further investigation is required to determine its true nature and history.
