The galaxy presents as a flattened, elliptical shape, with a noticeable bulge in the center. The core region exhibits a bright, yellowish hue, suggesting a concentration of older stars. Extending outward from the core, the galaxy displays a smoother, more diffuse structure with hints of reddish color on each end, likely due to dust absorption and potentially older stellar populations further away from the core. Overall, the morphology is relatively smooth, with no obvious spiral arm structures or major disturbances apparent. There is possibly a minor disturbance on one side. The galaxy's light profile appears to decline relatively gradually from the center outwards.
