The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. The core appears bright and yellowish-white, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes. The galaxy has a generally rounded shape, with a subtle elongation. No major disturbances or signs of ongoing merger activity are readily apparent in the image, with only minor asymmetries in the outer regions. The overall color profile indicates a relatively quiescent system, with low current star formation rate.
