The galaxy presents as a largely homogenous, elliptical structure. The light distribution is centrally concentrated, with a gradual falloff in surface brightness towards the outer edges. There is no discernible spiral arm structure or dust lane visible. The galaxy's color index indicates a population of older stars, likely dominated by redder, lower-mass stars. There is no strong evidence of ongoing, significant star formation. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or recent mergers. Its morphology suggests a relatively smooth and evolved system, consistent with an elliptical classification.
