The galaxy presents a largely elliptical morphology with a high degree of central concentration. The light profile appears smooth and centrally bright, indicative of an older stellar population dominating the overall luminosity.  A slight color gradient can be observed, with the core region appearing more yellow than the outer regions. The outer regions appear to fade gradually into the background. There is no visible evidence of spiral arms, dust lanes, or ongoing major mergers. Subtle variations in surface brightness suggest minor internal substructure, though high angular resolution data would be required to fully characterize these features. The apparent roundness indicates it is likely viewed close to face-on. Overall, the galaxy seems to be a relatively undisturbed system, possibly with little current star formation. 
