This galaxy presents as a somewhat smooth, elliptical-like structure with a notable central bulge. The core region exhibits a reddish hue, potentially indicative of an older stellar population or significant dust obscuration. Surrounding the core, a fainter, more diffuse halo is visible, displaying a greenish tint that may signify the presence of younger stars or ionized gas. No distinct spiral arms or bar structures are readily apparent, suggesting it is most likely an early-type galaxy. There is a slight distortion on one side of the galaxy, but overall the disk is largely undisturbed, with a small chance of it being in the early stages of a minor merger.
