The galaxy appears as a centrally concentrated, elliptical object with a smooth, relatively featureless light distribution. Its morphology suggests a classification leaning towards an elliptical galaxy, lacking the distinct spiral arms or bar structures typically associated with spiral galaxies. The galaxy's color appears generally redder, indicating an older stellar population and a lower rate of star formation. There is no obvious indication of recent or ongoing mergers, tidal tails, or other signs of significant gravitational interactions. The overall shape is close to round. The galaxy is observed at a distance where it is relatively small on the sky.
