The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall shape is more oblate than spherical, leaning towards an intermediate form between round and elongated. The color profile exhibits a yellowish core, which likely indicates an older stellar population dominating the central region. Surrounding the core, a blueish halo is present. There is no clear evidence of spiral arms or a well-defined disk, but a faint disk-like structure might be present. There are no major disturbances or signs of an ongoing merger evident from its morphology, although the galaxy does appear slightly disturbed.
