The galaxy presents a morphology suggestive of a recent or ongoing merger event. The primary galactic body exhibits a generally smooth profile, though there's evidence of tidal distortion. A secondary, smaller component is visible to one side, possibly a dwarf galaxy in the process of accretion or a remnant of a larger galaxy following a significant collision. The color distribution reveals a central concentration of older stellar populations, indicated by a yellowish hue. Patches of bluer light are observed primarily within the disturbed regions, indicative of ongoing star formation triggered by the interaction. The overall structure is somewhat amorphous, deviating from a clear spiral or elliptical shape. Faint tidal tails or extended stellar streams may be present, though their visibility is limited by the image resolution. 
