The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. Its color profile suggests a relatively homogenous stellar population, with a dominant yellowish-white hue at the core that seems to fade towards a redder tinge moving outward. No distinct spiral arm structures are discernible, nor is there any indication of a prominent bulge. There are no immediately obvious signs of recent major merger activity or significant tidal distortions. The galaxy appears to be a relatively quiescent system. Based on its smooth appearance, this object likely consists of old stars with very low star formation.
