The galaxy appears as a singular, moderately luminous object with a slightly ellipsoidal shape, indicating a possible classification as an elliptical galaxy. Its core exhibits a bright, concentrated intensity. There are faint, diffuse features that could be interpreted as the result of a past interaction or merger. The central region is predominantly yellow-orange, suggesting an older stellar population, with only minimal traces of bluer light. The overall structure suggests a system that has largely completed its major star formation epoch, with minimal indications of active ongoing star birth in the disk. Given that the galaxy is relatively smooth in appearance with very little sign of a disc, and its yellow-orange color, it suggests it has evolved into an early-type galaxy.
