The galaxy presents as a largely smooth, centrally concentrated object with a near-spherical morphology. The core exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. The outer regions display a gradual decline in surface brightness, transitioning to a faint, indistinct halo. There is minimal evidence of spiral arms or significant star formation regions within the galaxy's disk. Faint hints of blueish color, possibly indicating younger stars, are sparsely distributed in the outer regions, but this is not definitive. There is no clear evidence of significant tidal disturbances or ongoing merger activity. Overall, the galaxy appears to be a relatively quiescent, early-type system.
