The galaxy appears as a centrally condensed, luminous object, roughly elliptical in shape. The core exhibits a distinct yellowish-orange hue, potentially indicating an older stellar population. A surrounding, less intense halo displays a bluer tinge, which might suggest the presence of younger stars and ongoing, albeit low, star formation activity. The overall structure appears relatively smooth and undisturbed, with no obvious signs of spiral arms or major merger events. There might be subtle irregularities or minor disturbances in the outer regions of the halo, but the galaxy appears to be primarily relaxed in its structure.
