The galaxy presents as a relatively smooth, elliptical morphology. Its light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy appears mostly featureless, showing no prominent spiral arms or distinct structures. It exhibits a rounded shape, approaching circularity in its overall form. No signs of major mergers are apparent; however, there is a subtle indication of minor disturbances. The light from the galaxy has a reddish hue overall, suggesting an older stellar population with little ongoing star formation.
