The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a moderate axis ratio suggesting it is neither perfectly spherical nor highly flattened. There is a notable color gradient, with the core region exhibiting a yellowish-orange hue, possibly indicating an older stellar population or dust obscuration. Fainter, bluer light extends outwards from the central region, which could indicate more recent, but limited, star formation. No distinct spiral arms or other features are readily apparent, implying the light is primarily due to the bulge component. Overall the galaxy appears to be a quiescent system with moderate mass and low star formation rate.
