The galaxy presents a generally smooth morphology, with a high degree of central concentration. It exhibits a moderate yellow-red color profile, indicating a significant population of older stars. There is a subtle extension in one direction, suggesting a minor tidal interaction or possible disk-like structure. The galaxy's shape approximates a rounded form, deviating slightly from a perfect ellipse. There is no apparent sign of significant ongoing merger activity. The overall structure is that of a concentrated spheroid with a fading, diffuse outer halo.
