The galaxy presents as a relatively smooth, elliptical structure, possessing a high degree of central concentration. The core region exhibits a bright, intense luminosity, suggesting a high density of stars. Moving outward from the core, the light gradually diminishes, blending into a more diffuse halo. There appears to be minimal evidence of spiral arm structures or significant dust lanes. The overall color profile is suggestive of an older stellar population. Subtle variations in color within the galaxy, with a slightly bluer tint in the outer regions, hint at possible ongoing, though subdued, star formation activity. The galaxy displays a shape that is close to circular. There appears to be only minor evidence of galactic mergers or tidal disturbances.
