The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a nearly circular morphology, with only a slight deviation from perfect roundness. The light distribution suggests a centrally dominant spheroidal component. There is no obvious evidence of spiral arms or a prominent disk structure. The galaxy displays a color gradient, transitioning from a yellowish-white core to a bluer outer halo. While mostly smooth, there is a suggestion of subtle disturbances in the outer regions, perhaps indicative of minor interactions. Overall, the galaxy appears to be a mature system dominated by older stellar populations, with a mass that is relatively high and a SFR that is relatively low.
