This galaxy exhibits a disk-like morphology with a notable degree of disturbance. While a smooth component is present, there are clear features indicative of either spiral arms or tidal disruptions. There seems to be some ongoing or recent gravitational interaction. A faint and diffuse component surrounds the central structure, suggestive of a stellar halo or extended disk. The galaxy appears to be relatively blue, implying ongoing star formation. Some evidence of merging might be happening, but further observation is needed to confirm. 
