The galaxy appears to be a relatively smooth, elliptical galaxy, approximately 4 kpc in radius. Its morphology is characterized by a concentrated central bulge dominating the overall light profile. The isophotes are elongated, suggesting an intermediate ellipticity. There is no evidence of spiral arms or significant dust lanes. The color is generally red, indicating an older stellar population with suppressed star formation activity. The estimated mass of the galaxy is substantial, consistent with a mature elliptical galaxy. Based on its appearance, it does not appear to be undergoing any major mergers, though some minor disturbances cannot be ruled out.
