This galaxy appears to be a relatively smooth and rounded elliptical galaxy, exhibiting a concentrated central bulge that gradually fades outward into a less defined halo. The core displays a yellowish hue, likely indicative of an older stellar population. The outer regions show a slightly bluer tinge, potentially suggesting the presence of some younger stars or ongoing, albeit subdued, star formation activity. There appears to be only minor indications of a disk-like structure. No strong signs of tidal disturbances or merging events are immediately evident, suggesting a relatively undisturbed evolutionary history.
