The galaxy appears to be a relatively smooth, elliptical system, possessing a high degree of circularity. The galaxy exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. No prominent spiral arms or distinct features are observed. The galaxy exhibits a subtle reddish hue, indicative of an older stellar population with a low rate of current star formation. There is no evidence of any major ongoing merger activity, although subtle disturbances cannot be ruled out. Overall, this galaxy presents as a quiescent, evolved system.
