The galaxy presents a roughly elliptical morphology, appearing largely smooth and centralized. There is a distinct color gradient visible, shifting from a bluer hue in the central regions to a redder, yellower color towards the outer edges. The core exhibits a bright, relatively uniform intensity profile, suggesting a significant concentration of older stellar populations. While largely smooth, the galaxy does show subtle indications of minor disturbances or irregularities in its outer regions, possibly indicative of past interactions or mergers. There may be some tidal features such as faint plumes or asymmetries distorting the smooth shape of the halo. Overall, the galaxy appears as an early-type, relatively evolved system with some evidence of past or ongoing interactions affecting its overall structure.
