The galaxy presents as a slightly elongated, diffuse object. It exhibits a smooth, centralized bulge with a yellowish hue, suggesting a population of older stars. There is no clear evidence of spiral arms or significant dust lanes within the visible structure. The overall morphology appears relatively undisturbed, with no obvious signs of tidal features or ongoing mergers. The galaxy's color profile indicates a bias toward redder wavelengths, which is consistent with a more evolved stellar population and a relatively low rate of current star formation. The galaxy displays an elliptical shape.
