The galaxy appears as a centrally concentrated object with a generally smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicating an older stellar population. A diffuse halo surrounds the core, displaying a subtle color gradient from yellow-green closer to the center to slightly bluer tones in the outer regions. This suggests the presence of younger stars and potentially ongoing star formation within the galaxy, particularly at the periphery. There is no clear evidence of spiral arms or a prominent disk structure. The overall shape is close to circular, with a very slight elongation. No obvious signs of major mergers or significant tidal disturbances are visible, although subtle asymmetries in the halo cannot be entirely ruled out.
