The galaxy presents a generally smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, leaning towards a moderately rounded appearance. There is a slight color gradient, appearing more yellow at its core, suggesting an older stellar population concentrated centrally. The outer regions appear slightly bluer, potentially indicating a small amount of ongoing star formation. No distinct spiral arms or bar structures are apparent, which aligns with a classification as an early-type galaxy. There appears to be a minor, subtle disturbance in its structure, but no clear signs of a major ongoing merger event. The overall color indices suggest the galaxy has evolved to a fairly red stage, consistent with a substantial mass and relatively low star formation rate.
