The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile with a relatively round morphology. There is little evidence of spiral arms or significant dust lanes. The galaxy appears to be relatively isolated, showing little sign of ongoing or recent major merger activity. The overall color of the galaxy is consistent with a population of older stars. There is some evidence of recent star formation, but this is likely at a low level given the overall color and smooth appearance.
