The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The color profile appears generally yellow to orange, indicative of an older stellar population. There are faint hints of a disk structure, but it is not well-defined. No prominent spiral arms or dust lanes are discernible. The overall structure suggests a system that has undergone significant evolution, with reduced star formation activity. There may be minor disturbances indicating a possible gravitational interaction with another galaxy. The galaxy exhibits a nearly round shape.
