The galaxy appears as a relatively smooth, concentrated object with a nearly circular morphology. The central region displays a bright, somewhat diffuse glow, suggesting a concentration of older stars and possibly a supermassive black hole at its nucleus. There is a subtle color gradient across the galaxy, appearing slightly more yellow/red in the core, and more faint blue at its edges. This may be indicative of a reduced rate of on-going star formation in the galactic center. No distinct spiral arm structures or significant dust lanes are visible. The galaxy does not show any obvious signs of recent or ongoing major merger activity. It seems to be undisturbed and relatively isolated. Its overall appearance suggests an elliptical or lenticular galaxy, evolved and relatively quiescent.
