The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light profile. There's an absence of distinct spiral arms or a well-defined disk structure. The central region displays a concentration of light, suggesting the presence of a galactic bulge or core. Based on its morphology, there is a chance of a merging event in its past or even in progress. There is possible sign of disturbance due to gravitational interactions. The galaxy shows hints of a tidal tail. This suggests it may be interacting with another galaxy or has experienced a merger in its history.
