The galaxy presents as a somewhat smooth, elliptical-like structure, with no obvious spiral arms or bar. Its light distribution appears centrally concentrated, fading gradually towards the edges of the galaxy with a slightly oblate spheroidal shape. The galaxy's color indices suggest a population of older stars. There is no current merger activity that can be observed in the galaxy and no obvious disk like structure. There are a few faint indications of star forming activity, and the overall magnitude of the galaxy suggests that it is of intermediate mass.
