The galaxy appears to be an elliptical galaxy, with a smooth, concentrated light profile. It exhibits a cigar shape, with an apparent elongation. The core of the galaxy is bright and yellowish-white, suggesting an older stellar population. The color becomes slightly redder as it extends from the center, indicating the presence of aging stars. There is no obvious spiral arm structure or dust lanes visible, supporting the classification as an elliptical galaxy. There are no significant signs of disruption that would suggest recent major merger events.
