The galaxy presents a disturbed morphology, indicative of potential past or ongoing interactions. Its overall structure appears elongated, possibly a spiral galaxy viewed at an oblique angle. A brighter, more concentrated central region is evident, suggesting the presence of a galactic bulge.

Diffuse blue light is visible in the outer regions of the galaxy, hinting at ongoing star formation. Patches of redder light are also present, potentially indicating older stellar populations or regions of dust obscuration.

Overall, the galaxy exhibits a non-uniform distribution of light, with areas of varying color and intensity, which supports the idea of recent disturbances or mergers.
