The galaxy presents a largely smooth morphology, exhibiting an elliptical or lenticular form. The central bulge is prominent and generally circular. There may be some slight deviation from perfect circularity. The color gradient suggests a relatively older stellar population. There is little evidence of strong spiral arm structures or significant dust lanes. A slight color variation toward the outskirts hints at some ongoing, albeit subdued, star formation. The galaxy is likely relatively massive, potentially residing at the upper end of typical galaxy mass ranges. There is no distinct evidence of major ongoing merger activity, although the possibility of minor tidal interactions or past minor mergers cannot be completely ruled out.
