The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth and symmetrical morphology. The light profile appears to gradually decrease in intensity from the core outwards, lacking distinct spiral arm structures or a prominent bar. A slight elongation is observed, but overall, the galaxy appears to be close to round. Color gradients are subtle, with a marginally bluer central region transitioning to slightly redder outer regions. No significant dust lanes or tidal features are readily apparent, and the overall appearance suggests a well-mixed stellar population. The integrated light suggests a moderate level of star formation activity. The absence of major disturbances points towards a dynamically relaxed system, indicating that major merger events are unlikely to have occurred recently.