The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a primarily yellow-orange color, suggesting a dominant population of older stars. The luminosity profile appears centrally peaked, diminishing gradually toward the outer edges, with no clear indication of spiral arm structures. The isophotes appear relatively regular and elliptical, with a slight deviation, perhaps from a weak tidal disturbance or a minor interaction. The overall light distribution suggests a system undergoing or having recently completed a transition toward a redder, more quiescent state.
