The galaxy presents a generally smooth, elliptical morphology. It appears nearly circular in shape. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar population density, potentially indicative of an older stellar population and low levels of star formation. There is a slight color gradient from the center outwards, transitioning to a slightly redder hue in the outer regions. No obvious spiral arms or distinct features are discernible, and there is no apparent ongoing merger activity or tidal disturbances.
