The galaxy presents a largely smooth, elliptical morphology. A concentrated central bulge is clearly visible, appearing yellow in color, suggesting a population of older stars. There is a lack of prominent spiral arms or distinct features typically associated with disk galaxies. The light profile appears relatively smooth, without significant irregularities or tidal disturbances, though some subtle asymmetric features are present. Its overall structure implies a relatively evolved system, potentially indicative of minimal ongoing star formation. Based on the observed color and morphology, this galaxy is most likely a large elliptical galaxy with a significant population of evolved stars and low rate of star formation. 
