The galaxy exhibits a disturbed morphology, with an asymmetrical structure suggestive of an ongoing or recent merger event. A significant portion of the galaxy's light is concentrated in two distinct lobes, possibly remnants of the progenitor galaxies or tidal features resulting from their interaction. The color distribution within the galaxy appears non-uniform, with both reddish and bluish hues present. The reddish regions may indicate older stellar populations or dust obscuration, while the bluish regions could be associated with younger, hotter stars formed in bursts of star formation triggered by the merger. A faint, extended halo or tidal tail is suspected. The presence of significant merger activity could be influencing the overall star formation rate.
