The galaxy appears as a centrally concentrated, elliptical-like structure with a relatively smooth light distribution. The core exhibits a yellowish hue, possibly indicating an older stellar population. Fainter, less concentrated light extends outwards, transitioning to a slightly redder tone. There are no clear spiral arms, bar structures, or significant dust lanes visible. The morphology appears largely undisturbed, with no obvious signs of a recent major merger event or tidal interactions. The overall appearance is consistent with that of a relatively evolved galaxy.
