The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, appearing mostly round but trending towards slightly elongated. The light profile exhibits a radial gradient with a bright, yellowish core that gradually diffuses outwards into a fainter halo. There is no discernible spiral structure or prominent dust lane visible. The galaxy appears to be fairly isolated, lacking obvious signs of ongoing major mergers, although minor disturbances cannot be ruled out at this resolution.
