The galaxy presents as a relatively smooth, elliptical form. Its light profile appears centrally concentrated, with a gradual decrease in luminosity towards the outer edges. The core region exhibits a yellowish hue, potentially indicating an older stellar population dominating the center. Fainter, bluer regions are observed in the periphery of the galaxy, hinting at the presence of younger, hotter stars and some ongoing star formation. The overall morphology suggests a system that is not experiencing any major mergers or strong tidal disturbances, although subtle asymmetries could indicate minor interactions in its past or ongoing minor disturbances. The galaxy's elongated shape, but still relatively round, suggests it is somewhere between a perfectly spherical elliptical and a more flattened lenticular type.
