The observed galaxy presents a complex morphological structure, appearing to be the result of an ongoing or recent merger event. Two distinct, concentrated luminous regions are visible, suggesting the presence of two galactic nuclei in close proximity. The overall form is somewhat irregular and elongated, lacking a clear spiral or elliptical structure, and displays tidal features. The galaxy has a general yellowish hue, indicative of an older stellar population and relatively low ongoing star formation, although some bluer regions can be seen. 
