The galaxy presents as a relatively smooth object, likely an elliptical or lenticular galaxy at a considerable distance. Its core is a bright, concentrated region exhibiting a yellowish-orange hue, suggestive of an older stellar population. This central bulge gradually fades into a more diffuse halo. The halo appears slightly elongated, displaying a subtle disc-like feature along its major axis. There are hints of bluer, more recent star formation activity within the outer regions, indicating a low ongoing star formation rate. The galaxy does not appear to be undergoing any major mergers, although there may be some signs of minor tidal disturbances in the outer halo. The overall morphology suggests a galaxy that is evolving toward a more quiescent state.
