The galaxy presents a generally smooth, rounded morphology. There is a slight elongation, but it appears mostly circular. The light distribution is concentrated towards the center, indicating a possible bulge. There is minimal evidence of spiral arms or a distinct disk structure. The color appears relatively uniform across the galaxy, hinting at an older stellar population and a low star formation rate. Faint disturbances may be present, possibly indicating a past interaction. These features are subtle, implying that if there was a merger, it was likely minor.
