The galaxy presents as an elliptical morphology, appearing relatively smooth and concentrated. The light profile exhibits a strong central bulge, characterized by a high degree of symmetry and a lack of significant substructure. The color gradient suggests an older stellar population, with a pronounced concentration of redder hues towards the galactic center and a subtle shift to slightly bluer tones in the outer regions. There are no visible spiral arms or prominent dust lanes. The overall shape deviates slightly from a perfect circle, appearing somewhat elongated. There might be evidence of minor tidal disturbances or interactions with other galaxies. Overall, the galaxy appears to be a well-formed and relatively undisturbed system. It is likely a massive galaxy with a low star formation rate.
