The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core that diminishes gradually in intensity outwards. The overall color appears to be a blend of red and green hues suggesting an older stellar population with ongoing star formation. There is no apparent spiral structure or distinct disk features visible. The galaxy appears relatively isolated, showing no obvious signs of tidal interaction or major disturbances. There are no discernible irregular features, such as extended plumes or tails indicative of recent mergers. The shape appears to be quite circular.
