The galaxy appears as a fairly smooth, elliptical object, nearly circular in shape. It exhibits a dominant central bulge with a yellow-orange hue, suggesting an older stellar population. There is a smaller, less prominent region of redder emission offset from the center, potentially indicating a region of dust obscuration or a small area of ongoing star formation. No distinct spiral arms or strong tidal features are apparent. The overall light distribution is concentrated towards the center, fading gradually towards the edges. The relatively smooth morphology suggests a system that has undergone significant merging activity or has been quiescent for a considerable period. The colors indicate a red sequence galaxy with little ongoing star formation in most of the object. 
