The galaxy appears as a concentrated, centrally brightened structure. It exhibits a generally elliptical morphology, with a smooth, diffuse halo extending from the central bulge. The color profile shifts from a warmer, yellow hue in the core to cooler, reddish tones in the outer regions. There is no definitive spiral arm structure visible in the image, and the galaxy shows little evidence of irregular features, strong tidal disturbances, or an ongoing major merger event. There is a slight asymmetry, as the light is more diffused to the top of the image than the bottom, but not enough to definitively indicate a merger. The compact morphology and color gradient suggests an evolved system with a relatively old stellar population. Considering the observed smoothness and lack of prominent features, the galaxy is likely an elliptical, though it could be an early type spiral. The galaxy is of substantial mass, and has low star formation rates, and thus is likely a passively evolving system. 
