The galaxy presents as a relatively smooth, elliptical-like structure, with a centrally concentrated bulge. The core region appears yellowish-white in color, suggesting an older stellar population. Moving outward from the center, the galaxy transitions into a bluer halo. There appears to be a hint of a disk structure. There are no indications of strong spiral arm features, but some irregularities are present within the disk. No significant signs of on-going major merger activity are visible, although minor tidal disturbances cannot be ruled out.
