The galaxy presents as a moderately bright, relatively smooth object. It has a largely elliptical morphology, appearing mostly round with slight deviations. The central region displays a more concentrated and brighter luminosity. A subtle color gradient is observed, transitioning from a yellowish hue at its core to a bluish halo. This suggests a stellar population gradient, with older, redder stars concentrated centrally and younger, bluer stars populating the outer regions. Subtle distortions are apparent in the outer regions. Evidence of minor disturbances are visible, but no major ongoing merger is indicated.