The galaxy presents as a centrally concentrated, elliptical-like structure, exhibiting a relatively smooth light distribution. There is a dominant central bulge which appears nearly spheroidal. The color gradient transitions from a yellowish-white core to a reddish-tinged outer halo. Subtle hints of disturbances or minor asymmetries are visible in the outer regions, although the overall morphology suggests a system that has largely completed the process of hierarchical merging. The extended halo is faint and diffuse. Star formation appears low, contributing to the redder color indices. There is no clear spiral structure. The galaxy is likely a relatively massive, evolved system.
