The galaxy presents as a generally smooth, elliptical-like object with a concentrated central bulge exhibiting a yellowish hue. The overall morphology appears fairly regular with an absence of prominent spiral arms or significant dust lanes. There is some subtle indication of possible tidal features or a very faint, disturbed disk, extending from the main body of the galaxy. The radial color gradient suggests older stellar populations dominate within the central region, while bluer, potentially younger populations may be present in the outer regions, although these features are faint. There seems to be little ongoing star formation.
