The galaxy presents as a somewhat smooth, elongated structure with a distinct central bulge that exhibits a yellowish hue. The galaxy's disk appears to be viewed at a significant angle relative to our line of sight, resulting in its cigar shape. The overall light distribution suggests a relatively high degree of symmetry. The bluer colors on the outside of the disk may indicate areas of more recent star formation in the galaxy. There is no discernible sign of a major merger or significant tidal disturbances.
