This galaxy appears to be a merging system, exhibiting significant morphological disturbance. It presents with a somewhat smooth profile overall but shows features indicative of tidal interactions. There is evidence of minor tidal structures and possible bridges or tails. The galaxy displays an intermediate axial ratio, appearing neither perfectly round nor highly elongated. The central region exhibits a yellowish hue, perhaps indicating an older stellar population, while the outer regions display a bluer tint, which could represent ongoing star formation.
