The galaxy presents as a centrally concentrated object with a smooth, somewhat elliptical morphology. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. There is a subtle elongation, but the overall shape is close to round. No significant tidal disturbances, strong asymmetries, or signs of ongoing major mergers are apparent. The galaxy exhibits a generally homogenous color profile suggesting a more evolved stellar population across the galaxy. Subtle color variations suggest some low-level star formation may be present, but the overall rate appears modest.
