The galaxy appears to be an intermediate system, neither purely elliptical nor a well-defined spiral. Its overall form is somewhat irregular.

The light distribution suggests a central, relatively bright core region. Fainter light extends outward, forming a diffuse halo. The galaxy exhibits a blue tinge, suggesting the presence of relatively young, hot stars. There is faint evidence of asymmetry or possible tidal features, indicating a potentially ongoing or past interaction or merger event. The central region is dominated by a blue-white glow, suggesting some level of current star formation.
