The galaxy presents as a relatively smooth, elliptical structure. There is a concentrated central bulge of high luminosity, decreasing in brightness towards the outer edges. The shape appears more elongated than circular, tending towards an in-between or intermediate ellipticity. No significant dust lanes or spiral arm structures are discernible. There are no obvious signs of major disturbances or mergers. The overall visual impression is of a quiescent galaxy, likely dominated by an older stellar population.
