The galaxy presents as a singular, somewhat spheroidal entity with a smooth, largely featureless morphology. The light distribution appears centrally concentrated with a noticeable decline in intensity moving outward from the core, suggesting a dominant bulge component. There is a subtle color gradient within the galaxy, shifting from a slightly bluer hue in the outer regions to a redder tint towards the central core, indicative of potentially older stellar populations in the core and relatively younger stars towards the edges. Overall, this object appears to be a relatively massive galaxy at an intermediate redshift, potentially a massive elliptical galaxy or a lenticular galaxy viewed face-on. There might be a potential companion galaxy next to it. 
