The galaxy presents as a generally smooth, elliptical-like structure. There is a bright, concentrated central bulge that dominates the overall luminosity profile. The outer regions show a gradual fading in intensity, suggesting a relatively smooth distribution of stars. The color gradient indicates a redder core transitioning to slightly bluer outer regions, possibly due to variations in stellar populations or dust content within the galaxy. There's no immediately apparent evidence of significant spiral arm structures or major dust lanes, supporting the classification as a primarily smooth system. Minor asymmetry in the outer edges could indicate a past or ongoing minor interaction or tidal disturbance.
