The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that dominates the overall luminosity. The color profile suggests a population of older stars, leaning toward redder wavelengths in the central region. There's a subtle color gradient extending outwards, with the outer regions appearing slightly bluer. Evidence of a disk component is weakly present but not sharply defined. No major disturbances or signs of an active merger are apparent in the image. The galaxy exhibits a fairly high degree of symmetry.
