The galaxy appears to be a relatively compact, luminous object. It exhibits a generally smooth morphology, suggesting it could be an elliptical galaxy or a lenticular galaxy seen at a shallow inclination. The overall color profile leans towards the redder end of the spectrum, potentially indicating an older stellar population with relatively little ongoing star formation. There is a hint of some bluer light in the central region, which may indicate some younger stars are present in the nuclear region. The galaxy shows a subtle, elongated shape, and a disturbance is present within the central region. This could possibly be due to a minor merger event. No distinct spiral arms or other prominent features are clearly visible, and the galaxy seems to be in a relatively quiescent state.
