The galaxy presents as a spiral type, observed at a moderate angle relative to face-on. Two relatively distinct spiral arms are visible, originating from a central bar-shaped structure. The spiral arms appear somewhat patchy, indicating regions of active star formation. A small bulge is apparent in the center. Overall, the galaxy appears relatively undisturbed, without signs of a major merger or strong tidal interactions. The color suggests a moderate level of star formation activity with a well-defined disk structure.
