The galaxy presents as a centrally concentrated object, approximately circular in appearance, exhibiting a smooth morphology. A slight color gradient is visible, transitioning from a brighter, yellowish core to a redder, more diffuse outer region. No distinct spiral arm structures or dust lanes are discernible within the image resolution. The overall appearance suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy viewed face-on, with little ongoing star formation. There is no evidence of significant tidal disturbances or merging activity. The galaxy's light profile appears to be centrally dominant with a gradually decreasing intensity towards the outer edges.
