The galaxy presents a smooth, largely featureless morphology. Its light profile suggests a concentrated central region that gradually fades outwards, characteristic of an elliptical galaxy or the bulge component of a spiral. The shape appears to be largely rounded, deviating only slightly from perfect circularity. There is no strong evidence of spiral arms or a prominent disk structure visible in the available data. The galaxy exhibits a color gradient, with the central region appearing more yellow-orange, potentially indicative of an older stellar population. The outer regions are slightly bluer. There is no visible evidence of ongoing major mergers or strong tidal disturbances, but a minor asymmetry cannot be ruled out.
