The galaxy appears as a relatively small, disk-shaped system. There is a bright, concentrated central bulge. The bulge appears somewhat spherical and exhibits a blue hue. Surrounding the bulge is a flattened disk that is not particularly well-defined. Faint spiral arm structures may be present, but are not clearly resolvable. Overall the galaxy looks somewhat disrupted. There is a possible tidal tail extending from the left, which may indicate a past interaction or merger. The system's color gradient suggests active star formation in the disk, especially the central part of the disk.
