This galaxy appears to be a relatively large, evolved system exhibiting an elliptical morphology. It has a bright, concentrated central bulge, potentially indicative of a supermassive black hole or a dense stellar population. The bulge's color suggests a population of older, redder stars. The surrounding disk is not well-defined; a very smooth halo of bluer light surrounds the central bulge. Some areas appear to be slightly more separated and defined around the outside edges. There's no obvious indication of spiral arms. The overall color profile suggests moderate star formation activity with a prominent population of older stars. There is little evidence of any significant ongoing merger events or major disturbances to the galaxy's structure. 
