The galaxy presents a somewhat irregular morphology, displaying features that suggest it may be in a state of disturbance. A central, moderately bright region dominates the overall structure. The light distribution appears relatively smooth in the central region, but with subtle variations in color. There is evidence of blue-ish color, which could indicate the presence of younger stellar populations. The overall form lacks clear spiral arms or a well-defined disk, leading to the possibility that this is an elliptical galaxy or a galaxy undergoing a merger. Further investigation is needed to classify the morphological type.
