The galaxy presents as a single, relatively smooth, centralized object. The morphology appears to be elliptical, with a high degree of roundness. The core exhibits a strong concentration of light, suggesting a substantial bulge component.  The color profile indicates a population of older stars, leaning towards the redder end of the spectrum. There may be a slight indication of a minor disturbance in the galaxy's overall form, however, this is within normal levels. This object is a massive galaxy that is no longer forming many stars.
