The galaxy presents as a concentrated, centrally luminous object with a smooth, elliptical morphology. There is minimal discernible substructure, no spiral arm features or prominent dust lanes are visible, and it appears undisturbed with no major signs of ongoing merging activity. The light distribution appears to be relatively even, with a core that gradually fades out with increased radius. The light is reddish suggesting an older stellar population or the presence of dust, and the galaxy does not appear to be undergoing significant star formation. The isophotes are consistent with an ellipse that is nearly circular.
