The galaxy presents as a generally smooth, elliptical-like structure with a prominent central bulge. The core region displays a bright, concentrated luminosity, indicating a high density of stars. Moving outwards, the light gradually fades, revealing a somewhat diffuse halo. There is a subtle hint of a disk structure oriented almost edge-on; one side appears somewhat disturbed. The galaxy shows a redder hue in the central regions, transitioning to slightly bluer tints further out in the disk, which potentially indicates regions of ongoing, but minimal star formation. Based on its morphology, this galaxy is likely an evolved system with a substantial stellar mass and a relatively low star formation rate. Evidence suggests it may have experienced minor gravitational interactions in the past. The overall structure is primarily undisturbed.
