The galaxy presents a largely smooth, elliptical morphology. The central region is dominated by a concentrated, bright yellowish-white light, suggesting a substantial population of older stars. There's a gradual falloff in luminosity from the core to the outer regions, which are fainter and less distinctly colored. The overall form is nearly circular, with minimal indications of spiral arms or significant structural disturbances. This galaxy is likely a massive system. The absence of prominent blue regions indicates a relatively low rate of recent star formation. There may be minor signs of tidal disruption to the disk, but mostly presents itself as an undisturbed galaxy.
