The galaxy presents as a singular, centralized luminous structure. Its morphology appears largely smooth and featureless, lacking prominent spiral arms or a distinct disk. The shape is neither perfectly circular nor elongated, possessing an intermediate, somewhat irregular form. The central region displays a higher concentration of light, suggesting a possible galactic nucleus or bulge. There is a subtle color gradient visible, transitioning from a yellowish core to slightly redder outer regions, this may indicate variations in stellar populations or dust distribution within the galaxy. There are no obvious signs of ongoing major merger activity or significant tidal disturbances.