The galaxy exhibits characteristics of a major merger. It presents an irregular morphology with significant disturbances observed in its structure. Two distinct but closely interacting luminous components are visible, with a shared envelope of material suggesting ongoing tidal interactions. These components display a yellowish hue, potentially indicative of an older stellar population or dust obscuration. The overall shape deviates significantly from a smooth elliptical profile or a well-defined spiral structure, confirming the classification as a disturbed system. Faint tidal features may be present, but the resolution of the image limits further detailed analysis of these features. The galaxy appears to have a low star formation rate as indicated by the yellowish hue.
