The galaxy displays evidence of a recent or ongoing merger event. Two distinct components are visible. One component presents a relatively smooth, centralized concentration of light, indicative of an older stellar population or bulge region. The other component appears more diffuse and exhibits a bluer color, potentially signifying ongoing star formation within a disturbed disk structure.

Tidal features or extended arms are suggested, further supporting the presence of a gravitational interaction. There are some irregular features, possibly clumps of young stars or disrupted gas clouds. The system's overall morphology is significantly disturbed, deviating from a typical spiral or elliptical classification.
