The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. A gradual radial decrease in surface brightness is observed, extending outwards from a bright, unresolved core. There appears to be a slight elongation, though the overall shape is nearly circular. There is no apparent disk component. The color is largely uniform across the galaxy, with a subtle shift towards bluer tones in the central region. No distinct spiral arm structures, dust lanes, or active star-forming regions are visible. Any signs of galactic mergers or tidal interactions are not readily apparent.
