The galaxy appears as a moderately bright, elliptical-like object. It exhibits a smooth morphology with no distinct spiral arms or bars visible. The light distribution suggests a fairly uniform stellar population throughout its body, typical of an elliptical galaxy. A slight color gradient is observed, trending from redder hues towards the center to greener hues towards the outer edges. This may indicate a difference in stellar ages, with older, redder stars concentrated in the core and younger, bluer stars in the outskirts, though the limited resolution makes this difficult to confirm. There is no evidence of significant tidal disturbances or ongoing mergers.
