The galaxy presents as a predominantly smooth, elliptical structure. The central region exhibits a concentrated, bright core, appearing nearly spherical with a yellowish-white hue. Moving outward from the core, the light profile gradually fades into a more diffuse halo. The halo displays a slight elongation and is not perfectly symmetrical, with hints of a disk-like structure. Patches of greenish light are visible within the halo, which could indicate some regions of recent star formation. There appears to be very little visual evidence of strong spiral arm structures or significant dust lanes. There also appear to be no signs of any ongoing major merging events. The galaxy has a round, but not completely circular appearance. Any disturbances seem to be minor.
