The galaxy presents as a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge, appearing almost spherical. The color gradient indicates a transition from a yellowish-white core to a redder halo, suggesting an older stellar population dominating the outer regions. There is no readily apparent spiral structure or active star formation visible in this imaging, giving the galaxy a featureless and quiescent appearance. There is no evidence of any interactions or tidal distortions, nor any indication of dust lanes or prominent gas features. The overall impression is that of a well-evolved, relatively isolated galaxy.
