The galaxy presents as a centrally concentrated object with a fairly smooth, elliptical morphology. It is dominated by a bright, compact core of intense blue-white emission, which likely indicates a significant population of hot, young stars or possibly an active galactic nucleus. Moving outward from the core, a region of green-yellow emission surrounds the central area, transitioning to a diffuse redder hue at the periphery. The outer regions appear somewhat irregular and show subtle indications of possible tidal disturbances or interactions. The overall light distribution appears moderately concentrated, suggesting an intermediate Hubble type, with a slight indication of spiral arm presence. 
