The observed galaxy presents a somewhat irregular morphology. It displays a central, diffuse, and relatively brighter region. There are hints of a possible disk structure, although ill-defined, as well as signs of disturbances. The color appears to be primarily bluish-white, particularly in a few distinct concentrations or knots. There is a suggestion of possible minor interactions, as indicated by the perturbed structure. Further observation will need to be done to classify this further.
