The galaxy presents as a luminous, centrally concentrated object with a smooth and nearly circular morphology. The light distribution suggests a bulge-dominated system. There is minimal evidence of spiral arm structure or distinct features such as dust lanes. The galaxy exhibits a color gradient, appearing bluer in the outer regions and redder towards the core, indicating a potential difference in stellar populations. The estimated size suggests it is a sizable galaxy and based on its red color and bulge-dominated structure, it is most likely an elliptical galaxy. Based on color and smooth morphology, the star formation rate in this galaxy appears to be low. There is no strong evidence of any recent mergers or major tidal disturbances.
