The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is predominantly elliptical, appearing somewhat rounded in projection with only a slight deviation towards a more elongated shape. The light distribution is concentrated towards the center. The color gradient suggests a population of older stars, potentially indicating a lower current star formation rate. There is no discernible spiral arm structure or prominent dust lanes. A subtle color variation exists across the galaxy's profile, possibly indicating varying stellar populations or metallicity gradients. There is no evident signs of any major merger events happening. The structure appears undisturbed. 
