The galaxy presents as a centrally concentrated system with a smooth, diffuse light distribution. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population and potentially a prominent bulge component. This contrasts with the galaxy's outer regions, where a subtle blue tint is observed, possibly indicating the presence of younger stars and ongoing, although relatively quiescent, star formation. The galaxy appears largely undisturbed, lacking any distinct spiral arms, bars, or signs of major merging activity. The overall morphology is consistent with an elliptical or S0-type galaxy observed at a significant distance.
