The galaxy presents as a merging system, exhibiting significant morphological disturbance. A primary, centrally located mass of moderate size shows a diffuse, slightly elongated shape. Its core presents a yellow/white hue, possibly indicating an older stellar population, while the outer regions display hints of blue and green, suggesting recent or ongoing star formation. 

Attached to the central mass is an arm or tidal feature extending to the left of the image, exhibiting a more orange/red hue. This feature is less luminous than the core, hinting at lower stellar density or a population dominated by older, redder stars. The morphology strongly suggests a tidal interaction, possibly with a smaller galaxy that is not clearly resolved in the image or a more complex merger with multiple objects. The shape and color distribution points to an interaction that is past the initial contact phase, with evidence of tidal disruption and induced star formation.
