The galaxy presents as a single, centrally concentrated object with a relatively smooth appearance. Its overall shape tends towards round, displaying a degree of ellipticity but lacking any discernible spiral arm structure or a distinct disk component. There is no evidence of any major ongoing merging activity or significant tidal disturbances. Its size appears to be moderate, with light output strongest in the bluer wavelengths. Overall the mass of the galaxy appears to be consistent with a population of older stars. The star formation rate is fairly low.
