The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits a roughly elliptical morphology with a somewhat rounded appearance. There is a distinct color gradient, transitioning from a yellowish hue in the central region to a bluer, more diffuse outer halo. The smooth light distribution suggests an older stellar population, though the presence of bluer light in the outer regions may indicate some ongoing, albeit moderate, star formation activity. There is no apparent indication of strong tidal features, major disturbances, or a significant ongoing merger event. The overall structure implies the galaxy is relatively undisturbed and likely represents a mature system.
