The galaxy presents as an elliptical morphology, although some features suggest a possible disk component. Its overall structure is mostly smooth, and it displays a radial gradient with a concentrated, bright central bulge. The galaxy exhibits a subtle color gradient, appearing bluer towards the center and becoming redder in the outer regions. There may be some indication of minor disturbances in the outer regions, but no significant features such as tidal tails or clear signs of an ongoing major merger are immediately apparent.
