The galaxy presents as a relatively smooth, centralized elliptical type. Its morphology is generally round, exhibiting a slight elongation. The color gradient indicates a redder core, possibly indicative of an older stellar population and a lower rate of star formation. The outer regions appear slightly bluer, which may suggest a younger stellar population or some ongoing star formation. There are no visible spiral arms or distinct dust lanes, reinforcing its classification as an elliptical galaxy. No signs of major merging or tidal disturbances are immediately apparent.
