The galaxy presents a primarily smooth and centrally concentrated morphology. Its overall shape appears to be elliptical or lenticular. The light distribution suggests a relatively old stellar population, with the core appearing bright and gradually fading outwards. Some subtle structural features are present, indicating possible minor disturbances or ongoing interactions within the galaxy. The galaxy exhibits a bluish tinge around its edges, possibly indicating areas of younger star formation. The smooth nature of the light suggests that it is unlikely to be a spiral galaxy. The data points towards a galaxy that may be evolving gradually, experiencing minor internal disturbances rather than major mergers.
