The galaxy presents a generally smooth, elliptical morphology. A prominent central bulge region dominates the light profile, displaying a yellowish-white hue, potentially indicative of an older stellar population. Moving outward from the bulge, the light gradually fades into a more diffuse halo, with a subtle transition in color. There are very faint signs of possible disturbances, but no clear evidence of major mergers or tidal tails. The overall shape suggests a relatively evolved system, possibly nearing a state of quiescence. There are some hints of possible ongoing, very low-level star formation within the galactic disk and bulge.
