The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge. The light profile is centrally concentrated, diminishing gradually outwards. The central region appears yellowish-white, potentially indicative of an older stellar population. There is an extended, bluer halo, which could signify more recent star formation activity, though the smoothness suggests a lack of prominent spiral arms or distinct features commonly associated with ongoing star formation. The overall morphology indicates the galaxy is undisturbed, displaying no obvious signs of ongoing or recent merger events. The shape is mostly round.
