The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It is generally round with a slight deviation towards an in-between, less circular shape. There is no visible evidence of spiral arms or a prominent disk structure, instead presenting a featureless, smooth profile. The light distribution suggests a fairly old stellar population, with a dominant, centrally located bulge. No major merging activity or significant tidal disturbances are apparent. The overall color index appears to be relatively blue, suggesting a moderate amount of ongoing star formation for a galaxy of this type. Minor disturbances may be present, but are not immediately clear.
