The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a significant concentration of older stellar populations. Some disturbances are visible that could potentially suggest a minor merger event or ongoing tidal interactions. The galaxy's color profile indicates a redder overall hue, typical of galaxies dominated by evolved stars with reduced rates of active star formation. The overall structure appears relatively compact. There is a faint, diffuse halo surrounding the primary galactic body.
