The galaxy appears as an elliptical structure with a smooth and diffuse light distribution. There is an absence of prominent spiral arms or dust lanes. The galaxy exhibits an overall color gradient, with a brighter, more yellow core and a bluer, fainter halo or outer region. The elliptical shape of the galaxy indicates a lack of significant rotational support and suggests a dynamically relaxed system. The light profile indicates a concentration of older stars in the central region, and the apparent blue color of the halo region might suggest the presence of a younger stellar population there, with signs of recent star formation. The roundness is not significant. There do not appear to be any major mergers going on at this time. 
