The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The central region exhibits a yellowish hue, which may indicate an older stellar population. The overall light distribution appears relatively uniform, lacking any prominent spiral arms or distinct features. The galaxy's shape is generally round. There is no strong indication of significant ongoing star formation or major disturbances from potential mergers. Faint wisps or minor asymmetries are not entirely absent, hinting at potential interactions or past merger events.
