The galaxy presents as an elliptical morphology, exhibiting a concentrated central bulge. It has a golden hue, particularly concentrated towards the core, suggesting an older stellar population. The overall structure appears relatively smooth, lacking prominent spiral arms or distinct features. Faint extensions are visible, hinting at potential tidal interactions or minor disturbances. A slight asymmetry is observed, indicating it may not be perfectly relaxed and could have experienced past interactions or mergers.
