The galaxy presents as a relatively smooth, elliptical object. The light is concentrated towards the center, suggesting a prominent bulge. The color gradient suggests a primarily older stellar population. The galaxy appears somewhat elongated rather than perfectly circular. No distinct spiral arm structure is discernible; the overall texture is quite homogenous. There is no strong evidence of active star formation regions or significant dust lanes. There is no strong evidence for ongoing major merging activity, although some minor disturbances cannot be completely ruled out. The galaxy appears to be a relatively undisturbed system that is in a relatively relaxed state.
