The galaxy presents a primarily smooth morphology, with a high degree of central concentration. Its overall shape is somewhat elliptical, appearing nearly round. There may be some very subtle disturbances or features in the surrounding regions. The galaxy exhibits a color gradient, transitioning from a bright, yellow-white core to a reddish outer halo. This color suggests that the core may be dominated by older stellar populations, while the outer regions may contain a mix of intermediate-age and older stars. The light emitted by this galaxy indicates that the mass is very high but its star formation rate is relatively low. 
