The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. There is a noticeable radial color gradient, with a brighter, yellower core transitioning to a bluer outer halo. The overall shape is elliptical, appearing somewhat elongated but tending toward a more circular form. There is no obvious evidence of spiral arms, bars, or strong tidal disturbances. The galaxy appears isolated, lacking any prominent companion galaxies or indications of ongoing merger activity. The light distribution is relatively uniform, suggesting a well-mixed stellar population.