The galaxy presents as a complex morphological structure, exhibiting characteristics suggestive of an ongoing or recent merger event. A prominent feature is the presence of multiple distinct luminous components. One core exhibits a reddish hue, potentially indicating an older stellar population or significant dust obscuration. Adjacent to this, another bright core displays a yellowish-white color, which may signify a region of intermediate-age stars. A fainter, bluish component is visible on one side of the galaxy, which could indicate a region of active star formation. The overall shape is irregular, lacking the well-defined spiral arms or elliptical structure. The central bulge is not strongly defined, and there is evidence of tidal distortions and interactions between the merging components. These disturbances extend outwards, creating a diffuse halo of light.
