The galaxy presents as a relatively smooth, centrally concentrated object. Its shape appears to be somewhere between round and elliptical, with a slight elongation suggesting an oblate spheroidal structure. There is no obvious evidence of spiral arms or a distinct disk component. The galaxy exhibits a color gradient, transitioning from a brighter, yellower core to a bluer and fainter outer halo. The smooth morphology and color profile suggest a population dominated by older stars, with limited ongoing star formation. There are no signs of major tidal disturbances or ongoing merger activity in this image.
