This galaxy presents as a flattened, elliptical structure. There is evidence of a prominent central bulge with a diffuse disk.

The bluer hue at one end suggests an active star-forming region. The yellow-red color at the opposite end might indicate an older stellar population. The disk appears relatively smooth with subtle variations in brightness. Based on the elongation and lack of defined spiral arms, it appears as a lenticular galaxy. However, some disturbances in the disk are present. These disruptions could be the result of a minor merger or internal activity.
