The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, exhibiting a high degree of radial symmetry. The galaxy's light profile is dominated by a bulge-like component. There's a slight elongation, though it is difficult to tell if this is due to an edge-on disk. There is no apparent spiral structure or strong evidence of recent or ongoing mergers with other galaxies. The color suggests an evolved stellar population and is redder. There may be ongoing, but mild, star formation activity within the galaxy.
