The galaxy appears as a centrally concentrated object with a largely spheroidal morphology. The core exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. There's a relatively smooth and gradual decrease in surface brightness extending outward from the core. Faint reddish colors are visible in the outer regions, potentially indicating some ongoing, albeit low, levels of star formation or a population of red giant stars. No distinct spiral arm structure or pronounced dust lanes are readily apparent. The overall structure seems relatively undisturbed, with no obvious signs of major tidal interactions or recent merger events. Its fairly round appearance further reinforces the conclusion that this galaxy is primarily bulge-dominated.
