The galaxy presents as a primarily smooth, elliptical-like object. It exhibits a concentrated central bulge with a yellow-orange hue, suggesting a population of older stars dominating the core. The galaxy's light profile appears to fade gradually from the center outwards, with minimal discernible substructure or spiral arm features. A subtle greenish tinge is present in the outer regions, potentially indicative of some ongoing star formation. The overall morphology suggests a relatively evolved system, possibly an elliptical galaxy. There are only very minor signs of disturbances to the shape, no apparent merging events are occuring.
