The galaxy appears as a central, elliptical, and relatively smooth structure. It presents with a concentrated central bulge, exhibiting a slight elongation, and is generally uniform in color. The light distribution is more concentrated towards the center, diminishing towards the outer edges. There is no obvious spiral arm structure or dust lane visible, suggesting that the galaxy could be an elliptical type galaxy. There is no obvious ongoing major merging event; however, faint disturbances cannot be ruled out.
