The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color is predominantly yellow/gold, suggesting a population of older stars. The light is centrally concentrated, with a gradual falloff in intensity towards the edges. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy appears fairly isolated, with no immediate signs of tidal interaction or ongoing merger activity. The roundness suggests it is likely an elliptical galaxy viewed close to face-on, or potentially a spiral galaxy with a dominant bulge component.  The absence of blue color suggests that star formation rates are low to moderate.