The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology without prominent spiral arms or a well-defined disk structure. The galaxy possesses a bright, centrally concentrated bulge that graduates into a more diffuse outer halo. The color gradient indicates a population of older stars, as the central bulge is significantly redder than the outer regions, implying ongoing star formation. The overall shape of the galaxy appears elongated, suggesting a moderate degree of ellipticity. There is no visual evidence of major mergers or significant tidal disturbances.
