This galaxy appears to be a relatively smooth, centrally concentrated system. It has a slight elliptical morphology. The core exhibits a bright, yellowish hue. A diffuse, fainter halo surrounds the central region, exhibiting a subtle color gradient from yellow-greenish tones closer to the core to more bluish tones in the outer regions. There is no apparent dust lane or spiral arm structure visible in this image. The overall structure suggests a mature galaxy with a potentially quiescent star formation rate. No obvious signs of recent major merger events are observable, although subtle distortions or tidal features may be present at a level below the detection threshold. The overall color profile indicates a stellar population dominated by older stars.
