The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth appearance, suggestive of an early-type morphology. Its core exhibits a bright, yellowish-white hue, potentially indicating an older stellar population. Surrounding the core, a faint, diffuse halo of light extends outwards, becoming increasingly reddish with distance from the center. This may imply the presence of a gradient in stellar populations, with older, redder stars residing further out. There is minimal evidence of spiral arms or significant dust lanes, and the galaxy appears largely undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. A faint, subtle hint of bluer light is observed on one side, which may suggest localized star formation. The galaxy exhibits a nearly circular morphology, indicative of a relatively low inclination.
