The galaxy appears as a diffuse, irregularly shaped object. It presents a mottled texture, displaying variations in color and luminosity across its body. The overall hue is shifted towards the blue end of the spectrum in some parts, indicative of recent star formation. However, regions of redder coloration are also apparent, possibly signifying older stellar populations or dust obscuration. 

No distinct spiral arms or a well-defined nucleus are discernible. The light distribution lacks central concentration, suggesting a relatively low degree of symmetry. There is some evidence of disruption, possibly due to gravitational interactions, but no strong tidal tails or bridges are observed. The overall morphology of the galaxy could be classified as irregular. 
