The galaxy presents a largely smooth, elliptical morphology with minimal discernible features. The central region exhibits a bright, concentrated luminosity gradient, suggesting a prominent galactic nucleus. The light distribution indicates a high degree of central concentration. The overall color appears slightly redder, indicative of an older stellar population and suppressed recent star formation. There is little evidence of spiral arm structure or dust lanes. A very subtle hint of a disk-like structure is present, though not easily discernible. No major mergers or tidal disturbances are visible in this image. The shape approximates a circular form but is slightly elongated.