The galaxy presents as a relatively smooth, centrally concentrated light distribution, suggesting an elliptical morphology or a lenticular galaxy viewed face-on. The galaxy's core is bright and exhibits a yellowish-white hue, indicative of an older stellar population. This area appears to be spheroidal in shape.  

Moving outward from the core, the light gradually fades into a more diffuse halo.  There is a subtle hint of a disk-like structure, though it does not appear as a dominant feature. The outer regions show a bluer tint, possibly indicating some ongoing star formation. No strong signs of spiral arms or distinct features indicative of major recent mergers are apparent.  The galaxy appears largely undisturbed, with a high degree of central symmetry.
