The galaxy appears as a single, relatively smooth object. The light profile suggests a centrally concentrated bulge. Color gradients appear minimal, though the central region exhibits a slightly yellower, and thus potentially older, stellar population compared to the outer regions. The shape of the galaxy appears nearly circular. No obvious spiral arm structures are visible, nor are there any clear signs of tidal disturbances or ongoing mergers. The overall morphology is suggestive of an elliptical galaxy. The galaxy shows signs of limited star formation.
