The galaxy presents as a relatively smooth, centralized object, exhibiting a slightly elliptical morphology on the plane of observation. There is little apparent structure, such as spiral arms or a prominent bar. The color profile suggests a population dominated by older stars, trending towards redder wavelengths. There is some evidence of low levels of star formation activity, but the bulk of the stellar population appears quiescent. There is no strong indication of any recent or ongoing merger events.
