The galaxy presents as a relatively smooth object, elliptical in shape with a distinct central bulge. The bulge appears to be comprised of older stellar populations, indicated by its concentrated, yellowish-white color. Moving outward from the core, a fainter disk component is observed, also appearing smooth and without resolved spiral arms or distinct features. This disk component exhibits a slight bluer hue, implying the presence of younger stars and ongoing, albeit subdued, star formation. There's no obvious evidence of a major merger event or tidal disturbances affecting the galaxy's morphology, but it could potentially be undergoing a minor interaction given the slight irregularity observed in its outer regions. Overall, the galaxy is likely a massive, passively evolving system at a moderate redshift.
