The galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merging event. There is evidence of multiple distinct nuclei or density concentrations, suggesting the presence of at least two progenitor galaxies. One nucleus presents a reddish hue, potentially indicating an older stellar population or significant dust obscuration. Another nucleus appears bluer, which may signify ongoing star formation.

Extending from these nuclei are faint tidal features or streamers of stellar material. These structures are indicative of gravitational disruption caused by the interaction. A significant portion of the galaxy appears relatively smooth and undisturbed, suggesting that the interaction may be in a relatively early stage. Some regions show a mottled appearance, possibly due to dust lanes or irregular star formation regions. Overall, the galaxy presents a disturbed morphology with signs of ongoing or recent merger activity.
