The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards from the core. There's a subtle color gradient; the central region exhibits a yellowish-white hue, suggestive of an older stellar population, transitioning to a slightly redder color in the outer regions. No distinct spiral arms or prominent dust lanes are discernible. The overall form is suggestive of an evolved system with a likely suppressed star formation rate. No signs of recent major merger activity or significant tidal distortions are apparent. The galaxy appears well-defined and isolated.
