The galaxy presents as a moderately luminous object with an apparent disturbed morphology. There is a bright central region, appearing nearly spherical, with a significant extension of diffuse material extending away from it. This extended structure is irregular, suggesting ongoing interactions or tidal disruption. The colour profile indicates a mixed stellar population, with hints of younger, bluer stars in the outer regions. Overall, the galaxy appears to be undergoing or have recently undergone a significant interaction or merger event. The galaxy appears to be neither completely smooth nor entirely disk-like, but rather a hybrid of both.
