The galaxy presents a relatively smooth and concentrated morphology. The light distribution suggests a centrally dominant bulge with a high degree of symmetry. The shape of the galaxy is somewhere between round and elliptical, appearing more elliptical. There is no clear evidence of spiral arms, a prominent disk, or significant dust lanes. The galaxy exhibits a color gradient, with the core appearing more yellowish-white, potentially indicating an older stellar population in the central regions. The outer regions appear somewhat fainter and slightly redder. There is no obvious sign of any major tidal disturbances or ongoing merger activity, though a very slight irregularity in the outer envelope of the galaxy cannot be ruled out with certainty. 
