The galaxy presents as a relatively large, well-defined elliptical or lenticular structure. It exhibits a smooth, centrally concentrated light distribution, with a bright, somewhat indistinct nucleus. There's a subtle color gradient, with the central regions appearing slightly more yellow/orange, possibly indicating an older stellar population and a reduced rate of star formation. Faint disk-like structures are visible, marked by slight hints of spiral arms. The absence of pronounced dust lanes further implies a diminished reservoir of interstellar medium, characteristic of later-type galaxies with a stellar mass on the order of 10^11 solar masses. Overall, the morphology suggests a galaxy that is largely quiescent in terms of star formation, with no signs of significant ongoing merger activity or major disturbances to its structure.
