The galaxy presents as a relatively smooth, elliptical-like structure with a discernible major axis. Its morphology suggests a possible classification as an elliptical galaxy or a lenticular galaxy seen at an angle. The central bulge exhibits a concentrated, bright, yellowish-white hue, indicating an older stellar population. Moving outward from the core, the galaxy gradually fades in intensity. There's a subtle color gradient, transitioning to more reddish tones in the outer regions, which could signify regions of slightly younger stars or dust obscuration. There is no apparent active star formation. The outer edges of the galaxy appear diffuse and ill-defined. Overall, the galaxy appears undisturbed.
