The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears primarily elliptical or spheroidal. The overall color profile indicates a relatively red population, suggesting an older stellar population. The light distribution is largely uniform, with a slight radial decrease in intensity from the center outwards. The galaxy appears largely undisturbed, showing no obvious signs of ongoing major mergers, tidal tails or significant disk component. The core shows a concentration of yellow light, suggestive of an older generation of stars. There are also hints of less concentrated star forming regions.
