The galaxy presents as a single, relatively smooth object, but close inspection reveals potentially two or more distinct nuclei or concentrations of light within a common halo. The object exhibits a largely elliptical morphology, with a high degree of central concentration in each of the light concentrations. There are few discernable features associated with spiral arms or a distinct disk structure. 

The galaxy's color index indicates a population of older stars, a minimal amount of dust, and a low rate of active star formation across the galaxy's entirety. There are no prominent features indicative of a highly disturbed system; however, there may be minor distortions or asymmetries in the outer isophotes potentially indicating an ongoing or recent merger event. The galaxy is of significant luminosity and estimated mass.
