The galaxy presents as a spiral type, viewed at a significant inclination. The central bulge appears luminous and concentrated. The disk is clearly visible, exhibiting a flattened shape, and displays some texture suggestive of spiral arm structure. The outer regions of the disk appear less defined. The overall color is a bluish hue, likely indicating the presence of younger stars, while the galaxy is also quite dim. There are subtle color variations visible, with some possible features in the disk indicating regions of active star formation. The galaxy displays no obvious signs of a major ongoing merger, but appears somewhat disturbed.
