The galaxy presents as a single, smooth, and concentrated body with a distinct spheroidal morphology. It exhibits a dominant central bulge that appears yellowish-orange. The surrounding region appears fainter, and bluer. No distinct spiral arm structure or obvious dust lanes are discernible in this image. Overall, the galaxy's color is consistent with an aging stellar population and a relatively low ongoing star formation rate. The galaxy appears undisturbed, with no signs of major mergers or significant tidal interactions. A subtle asymmetry or minor perturbation in the outer regions cannot be ruled out based on this image alone.
