The galaxy exhibits a morphology consistent with an edge-on disk galaxy. The overall shape appears flattened and elongated, viewed nearly perpendicular to its plane of rotation. The central bulge is not prominent. Evidence of internal structure, such as spiral arms, is not readily discernible from this viewing angle. There does appear to be a slight warp. There are no strong signs of recent major merger activity or tidal disturbances in the immediate vicinity of the galaxy. The galaxy appears smooth and undisturbed. The color suggests some star formation present, as indicated by the faint blue hue, but may be mostly quiescent.
