The galaxy presents as a relatively smooth, elliptical form. There is a clear concentration of light towards the galactic center, exhibiting a bright, yellowish core. The overall color suggests a more evolved stellar population, leaning towards older stars. The galaxy appears fairly round, showing only slight deviations from a perfect sphere. There are no obvious signs of ongoing major mergers, although subtle asymmetries might suggest minor gravitational disturbances or past interactions. There is a faint disk around the central bulge. The galaxy's extended halo is relatively uniform. There are no prominent dust lanes or spiral arm structures visible.
