The galaxy exhibits a somewhat amorphous morphology, lacking a well-defined spiral or elliptical structure. The light distribution suggests multiple, ill-defined components or clumps, potentially indicating ongoing or recent merger activity. There's an irregular distribution of light, with evidence of both bluer and redder components. The overall color profile suggests intermediate stellar populations. Patches of bluer light hint at regions of recent star formation. The spatial extent indicates a galaxy of considerable size, although the absence of clearly defined structures makes precise classification challenging. The morphology hints at a system far from dynamical equilibrium, possibly a product of significant gravitational interaction.
