The galaxy presents as a centrally concentrated, relatively smooth object, exhibiting a flattened, elliptical morphology. The color profile suggests a dominant older stellar population, with a yellowish-white core that gradually fades into a bluer halo. There appears to be minimal evidence of spiral arm structure or prominent dust lanes, lending to its smooth appearance. There's a slight asymmetry in the outer regions, hinting at a potential past interaction or minor disturbance. The overall impression is that of a galaxy that has largely exhausted its gas supply, resulting in a low rate of current star formation.
