This galaxy presents as a relatively smooth and concentrated object. It exhibits an overall elliptical morphology, deviating slightly from a perfect circular shape. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The color profile suggests a dominant population of older stars, evidenced by its redder hue. There is a possible minor visual disturbance in the symmetry of the galaxy indicating a very minor interaction with another galaxy. It is possible the galaxy is currently undergoing relatively low rates of star formation. The overall structure indicates a system that is relatively evolved.
