The object appears to be a relatively compact galaxy of moderate size. Morphologically, the galaxy appears to possess a smooth structure, with no clearly defined spiral arms or bar features. The light distribution indicates it is likely an elliptical galaxy or potentially a lenticular galaxy seen at a high inclination. There might be some faint disturbances in the galactic structure possibly indicating a minor ongoing merger or tidal interaction but is not major. The color indices suggest a relatively red galaxy, indicating an older stellar population or significant dust extinction.
