The galaxy presents a smooth, elliptical morphology. Its light profile exhibits a concentrated central bulge, which decreases gradually with radius. The color appears homogenous, tending towards a yellowish hue, indicative of an older stellar population. There is no evidence of spiral arms or a disk-like structure. The overall shape is largely spheroidal, with a slight elongation. There is a small sign of minor disturbances with no distinct signs of mergers.
