The galaxy presents a generally smooth and rounded morphology, exhibiting a dominant central bulge. There is faint hint of a disk-like structure. Its color appears primarily yellow-orange, suggesting an older stellar population. There is no evidence of spiral arms or significant dust lanes, although the edges are diffuse. The lack of distinct features suggests a relatively evolved system, potentially an elliptical or lenticular galaxy. There may be ongoing, but low, levels of star formation. There is no indication of tidal disturbances or major ongoing mergers.
