The galaxy presents as a fairly smooth elliptical morphology, exhibiting a concentrated central bulge that gradually diffuses outwards into a more extended halo. The light distribution is dominated by redder hues, suggesting an older stellar population. The galaxy appears relatively undisturbed with no obvious signs of recent major mergers or tidal interactions. There is slight flattening, but the overall shape is close to circular. A low level of ongoing star formation is suggested by the light in the bluer bands in the image.
