The galaxy presents a generally smooth, elliptical morphology with no immediately apparent spiral arm structures or significant dust lanes. The light distribution appears centrally concentrated, with a gradual decline in surface brightness moving outwards from the core. The galaxy exhibits a color gradient, transitioning from a brighter, yellower core to a slightly redder, more diffuse halo region. The overall color suggests an older stellar population is dominant, with potentially low levels of current star formation. There is no obvious evidence of ongoing major merger activity, although subtle distortions may be present upon closer inspection, potentially indicating minor interactions. The galaxy's apparent shape is somewhat elongated but close to a sphere, appearing more as an ellipse.
