The galaxy presents an overall elliptical morphology, although not perfectly spherical. The central region exhibits a high surface brightness, appearing nearly unresolved and intensely luminous, suggesting a possible active galactic nucleus or a dense concentration of stars. The light from the galactic center seems to dominate, giving the galaxy a very bright core.

Moving outwards from the center, the galaxy displays a gradual decrease in luminosity. The isophotes appear fairly smooth and regular, indicating a lack of major disturbances or recent merger events in the system’s history. The outer regions appear somewhat elongated, giving the impression of a slightly flattened spheroidal shape.

There is evidence of a subtle color gradient, where the central region displays a bluer hue, contrasting with the outer halo which appears redder. This may indicate different stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars predominating in the outer regions. There is an interesting, distinct redder region that is just off-center of the galaxy. It does not appear to be part of the overall spheroidal shape. This could be a distinct star forming region or area of dust obscuration. 
