The galaxy presents as a generally smooth, elliptical-like structure. A bright central bulge is clearly visible, exhibiting a concentrated luminosity. Moving outward from the core, the light gradually diffuses, creating a halo effect. The galaxy appears to be generally smooth, with some subtle indications of potential disturbances or faint disk-like features in the outer regions, although these are not sharply defined. There may be some minor ongoing gravitational interactions. The object does not appear to be a late-stage merger, but is likely an early stage merging galaxy. 