The galaxy presents as a diffuse, centrally concentrated object. The color profile suggests a somewhat evolved stellar population, leaning towards redder hues, indicative of older stars. The overall form appears mostly smooth, without a prominent disk or spiral structure immediately evident. While the core is relatively bright, the galaxy appears to be fading towards its edges with no sign of active star formation. Its shape is approximately in between round and elliptical. There are no obvious signs of a recent major merger, though a minor interaction with a smaller object can not be ruled out based on this image alone.
