The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish hue, suggesting an older stellar population. A fainter, more diffuse halo surrounds the core, with a subtle gradient in color, transitioning to a slightly bluer tint in the outer regions. This could potentially indicate the presence of younger stars or ongoing star formation, albeit at a relatively low level. No distinct spiral arms or prominent dust lanes are visible. The overall structure implies a gravitationally relaxed system that has likely undergone significant evolutionary processing.
