The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light distribution suggests a high degree of radial symmetry, with a gradual decrease in intensity from the core to the outer regions. The galaxy's color profile shows a relatively uniform distribution across the visible spectrum, lacking prominent blue star-forming regions or distinct dust lanes. The apparent lack of structural features, such as spiral arms or bars, is consistent with a spheroidal system dominated by an older stellar population. There is a slight color gradient from the center outwards to the outer halo with the halo appearing to be slightly redder than the central bulge. There is no indication of major tidal disturbances or interactions.
