The galaxy presents as a somewhat disturbed spiral or disk galaxy, possibly undergoing a minor or major merger, or showing signs of tidal disruption. The central bulge is prominent with an orange hue indicating an older stellar population. The disk appears to have a bluish color suggesting regions of active star formation. The overall shape is distorted, showing asymmetry on either side of the central bulge, with faint but discernible features hinting at possible tidal tails or disrupted spiral arms. It is oriented at an angle, not quite edge-on, but with enough tilt to give a sense of a flattened disk-like structure. Some regions within the disk appear relatively smooth while others show hints of substructure.
