The galaxy presents as a centrally concentrated, luminous object. Its morphology appears largely smooth, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a spheroidal shape, possibly elliptical. Color gradients within the galaxy indicate variations in stellar populations, with a yellowish hue near the core that transitions to a slightly bluer periphery, hinting at younger stars forming in the outer regions. There is no visually apparent evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's overall structure.
