This galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology is dominated by a bright central bulge with a soft, diffuse halo extending outwards. The light distribution suggests a high degree of symmetry, with a slightly elongated shape, but not heavily cigar-shaped. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a subtle color gradient, with the central bulge appearing more yellow-white, potentially indicating an older stellar population, and the outer regions exhibiting a bluer hue, possibly indicating the presence of some younger stars, although star formation is not prominent. Overall, the galaxy appears to be relatively isolated and undisturbed, showing no obvious signs of tidal interactions or recent merger events.
