The galaxy presents a largely smooth, elliptical morphology. Its light distribution is highly concentrated towards the center, indicative of a substantial central bulge. The galaxy's shape is close to circular. There is no clear evidence of spiral arms or a distinct disk structure. There are no obvious signs of tidal disturbances or ongoing major merger activity, although subtle asymmetries cannot be entirely ruled out. Colors are slightly bluer than usual in elliptical galaxies, indicating there may be some star formation present. The estimated physical size is a few kiloparsecs.