The galaxy exhibits a dominant, centrally concentrated bulge. This bulge appears relatively smooth and featureless with a yellow-white hue. Extending from one side of the bulge is a distinct, irregular feature. This feature shows a bluer color, hinting at the presence of younger stellar populations. The structure is somewhat diffuse and appears to be undergoing some form of tidal disruption or interaction, with some knotty areas. Overall, the galaxy appears to be undergoing a merger or strong interaction.
