The galaxy presents as a somewhat diffuse and irregular structure. It does not exhibit a clear, well-defined disk or spiral arms. There are hints of disturbed morphology, possibly indicative of ongoing or recent gravitational interactions. The light distribution appears uneven, with some clumpy regions suggestive of active star formation or dust obscuration. There is no central bulge apparent. The overall color suggests a mix of stellar populations, with bluer regions indicating younger stars and redder areas potentially indicating older populations or dust. The apparent lack of a distinct nucleus or bulge, along with the irregular shape, may classify this as an irregular galaxy, possibly undergoing a merger or experiencing significant tidal disruption.
