The galaxy appears to be a relatively smooth and centrally concentrated system. The light profile suggests an elliptical morphology, with no distinct spiral arm structures visible. The galaxy exhibits a yellowish-white color, indicating a likely older stellar population with fewer young, massive blue stars. There are no obvious signs of ongoing major merging activity, though there might be some minor asymmetry to the outer halo suggestive of past interaction. Based on the lack of blue light, the galaxy may have a relatively low star formation rate, which would be consistent with a more evolved elliptical type. The generally round shape further supports the possibility of being an elliptical galaxy, rather than a disk-dominated spiral seen at an angle.
