The galaxy presents a generally smooth and elliptical morphology. Its color profile exhibits a centrally concentrated yellowish hue, suggesting an older stellar population dominating the core. Fainter, bluer regions appear toward the periphery of the galaxy, possibly indicating some low-level star formation in the outer disk. There appears to be a slight asymmetry in the galaxy's shape, but no strong tidal features or obvious signs of a recent major merger are present. The galaxy is moderately bright. Overall, the galaxy appears as a typical, relatively undisturbed elliptical system with some evidence of ongoing, albeit limited, star formation activity.
