The galaxy exhibits an overall irregular morphology, suggesting a dynamically active state. Two distinct components are visible: a brighter, bluer region and a fainter, redder region. The blue component appears relatively smooth, possibly indicative of a spheroidal structure or bulge. The red component displays a more diffuse and less defined structure, potentially representing a disrupted stellar population or dust obscuration.

The color gradient across the galaxy suggests varying stellar populations and/or dust content. The bluer region is likely dominated by younger, hotter stars, while the redder region may contain older, cooler stars and/or significant dust absorption. The relative proximity and disturbed morphology of the two components strongly imply an ongoing or recent interaction or merger event. The shape is more "in between" round and cigar. The overall impression is one of a system undergoing significant tidal disruption and transformation.
