The galaxy appears to be an elliptical type, characterized by a largely smooth, concentrated light profile. The color is predominantly yellow-orange, suggesting an older stellar population with fewer young, hot stars. The galaxy has a moderately high degree of roundness, showing no distinct spiral arm structures. There is a faint feature extending from the main body on one side, potentially indicating a tidal tail or minor disturbance, possibly a result of a past interaction or merger event. The central region is more luminous, indicating a higher stellar density towards the core. Given the overall smooth and centrally concentrated morphology, the galaxy does not display characteristics of active star formation regions.
