The galaxy displays a complex morphology, indicative of an ongoing or recent merger event. There is a bright, somewhat spheroidal component exhibiting a reddish hue, possibly indicating an older stellar population or significant dust obscuration. Adjacent to this, another distinct, bluer component is visible. This bluer region is less defined, suggesting a more active star formation phase. The overall structure of the galaxy is irregular, lacking a clear spiral or elliptical shape. There are faint tidal features or disturbed structures extending from the core of the galaxy, further supporting the merger hypothesis. These features are subtle, indicating that the interaction may be in its later stages.
