The galaxy presents as a somewhat irregular structure. It appears to be undergoing a merger, or at least a significant interaction, indicated by its disturbed morphology. There is some visible distortion in its overall shape; it is not a perfectly smooth or elliptical object. Patches of blue color suggest regions of active star formation, perhaps triggered by the interaction. A more centrally located region exhibits an orange hue, indicating an older stellar population. Overall, this galaxy appears to be an intermediate-mass galaxy currently experiencing, or recently having experienced, a period of heightened star formation activity.
