The galaxy presents as a single, relatively smooth object with a concentrated central bulge. It exhibits a generally elliptical shape with a high degree of circularity, appearing mostly round in projection. The light distribution is dominated by redder hues, suggestive of an older stellar population and lower ongoing star formation. There is no discernible disk component or spiral arm structure visible. No significant tidal features or signs of major mergers are apparent in the image, though subtle indications of minor disturbances cannot be ruled out.
