The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a high degree of roundness. There is little evidence of spiral arms or a distinct disk structure. The galaxy displays a color gradient, transitioning from a reddish hue in the central region to a bluer hue in the outer regions. This suggests a population of older stars concentrated in the core, with relatively younger stars inhabiting the periphery. There is no obvious indication of ongoing major merger activity or significant tidal disturbances.
